00 00.2 -25 19 COO 273 Proper motion of B -025 -029. 00 00.4 +60 26 STI 1248 Proper motion of B +026 +010. 00 00.6 -52 38 FIN 294 Spectrum: K1/2III+A/F. 00 01.1 +69 35 STT 253 B is BD+68@1417. Proper motion of B +005 000. 00 01.1 -23 26 LDS 2070 B is CD-24@17944. 00 01.3 +60 21 STT 254 A is the semiregular variable WZ Cas. 00 01.3 +07 42 DU 4 Proper motion of B -035 -076. 00 01.3 -70 12 GLI 290 B is CPD-70@3035. Proper motion of B +056 -021. 00 01.4 +39 37 HLD 60 P = 227yr., a = 0.85", motion retrograde. 00 01.6 +64 37 MLR 79 Misidentified by Muller as BD +63@2093. 00 01.8 -25 48 B 630 Measures uncertain, too close. 00 02.2 +27 05 BU 733 85 Peg. P = 26.3yr., a = 0.83", motion direct. 00 02.3 -29 43 B 631 Zeta Scl. The companion is very faint and not accurately measured. A is a spectroscopic binary. 00 02.4 +10 47 A 1249 Too close 1940, 1947. 00 02.6 +66 06 STF 3053 B is BD+65@1988. Proper motion of B +004 -003. 00 02.6 -08 29 A 428 P = 218yr., a = 0.36", motion retrograde. 00 02.7 +59 58 ARG 47 Proper motion of B -004 -004. 00 02.8 +80 17 STF 3051 Proper motion of B +021 +021. 00 02.9 +71 22 STF 3052 Proper motion of B -007 +006. 00 03.1 +08 16 STF 3054 Proper motion of B -032 -033. 00 03.2 +45 08 HJ 1927 Proper motion of B +004 -022. 00 03.9 +27 59 A 429 Proper motion of C -003 -008. 00 04.0 +41 13 H 69 H IV 69. With error of 1@ declination it would be the same as STF 3064 rej. BDS 8. 00 04.2 +62 17 S 838 9 Cas. B is BD+61@2585. 00 04.6 +42 06 CHR 122 B is a spectroscopic binary. Hence the system is quadruple. 00 04.7 +35 47 HU 800 Round 1944, 1951- 1957. Motion in separation, with little angular change. 00 04.8 +38 10 BU 862 P = 403yr., a = 0.74", motion direct. 00 04.9 +58 32 STF 3057 Called a two-spectrum spectroscopic binary in the Bright Star Catalogue Supplement. 00 05.2 +30 20 STF 3058 Proper motion of B -041 -025. 00 05.4 +16 20 STT 255 B is BD+15@4934. Proper motion of B is +005 -028. 00 05.5 +34 06 HU 1201 A possible close approach about 1980. 00 05.7 +45 49 STT 547 Premature orbits have been computed. Motion direct. Both A and B have variable radial velocity. C has common proper motion. 00 05.7 +17 50 STF 3061 Proper motion of B +046 -017. 00 05.9 +18 05 STF 3060 Proper motion of B -137 -135. 00 06.3 +58 26 STF 3062 P = 107yr., a = 1.43", motion direct. One component is variable, P = 1.08 d, probably due to partial eclipses. It is designated V640 Cas. 00 06.3 -49 05 HDO 180 A is a spectroscopic binary. 00 06.5 +01 55 HJ 1000 Proper motion of B +040 -073. 00 07.8 +57 23 HJ 3241 HJ 1935. Proper motion of B 000 -005. 00 08.0 +31 23 STT 256 B is BD+30@3. The pair is, however, optical. 00 08.3 +20 29 BOW 3 Greenwich gives BD+19@5. J gives BD+19@2. Used ADS position. 00 08.4 +29 05 H 32 H V 32. Alpha And. A is a spectroscopic binary, P = 96.7d. Proper motion of the optical companion, B, -004 -024. 00 09.0 -54 00 HDO 181 Spectroscopic binary. 00 09.1 +59 38 ARG 1 B is BD+58@4. Proper motion of B +011 +019. 00 09.2 +59 09 AGC 15 Beta Cas. The primary is a Delta Scuti-type variable. Spectroscopic binary, P = 27 d. 00 09.3 +79 43 STF 2 P = 456yr., a = 0.92", motion retrograde. 00 09.4 +63 57 BUP 1 V641 Cas, a VV Cep-type system. 00 09.4 -27 59 BU 391 Kappa (1) Scl. 00 09.6 +38 26 PTT 1 This appears to be the same as ALI 473. PTT position 00 10.0 +38 23. 00 09.8 -33 47 SEE 3 P = 425yr., a =1.11". 00 09.9 +11 25 HJ 1939 Proper motion of B -015 -005. 00 09.9 +08 27 STF 4 Proper motion of B -004 -008. 00 10.0 +46 23 STF 3 A small star in field: 1831.33 133.0@ 4.57" (HJ). Possibly an illusion. 00 10.0 +11 09 STF 5 34 Psc. 00 10.2 +75 07 HJ 1938 Proper motion of B -001 +001. 00 10.4 +49 52 ES 2576 B is BD+49@17. Proper motion of B +006 -003. 00 10.6 -73 13 I 43 There is a long gap (1931-1977) in the observations. 00 10.7 +67 09 ES 114 Proper motion of B +016 +013. 00 10.7 +54 53 WOR 37 SX Cas, an eclipsing and spectroscopic binary, P = 36.6d. Spectral types A6shell and K3III. 00 10.9 +67 15 ES 113 Proper motion of B -013 +019. 00 11.2 +49 33 ES 2577 B is BD+48@28. Proper motion of B -002 -005. 00 11.5 +29 49 MLB 441 Proper motion of B +044 -001. 00 11.6 -27 48 LDS 2099 Kappa (2) Scl. 00 12.1 +53 37 CHR 1 Aa. Rapid motion, particularly in separation. BU 1026 Aa-B. P = 66.8yr., a = 0.251", motion direct. 00 12.2 +46 47 A 802 Not seen 1950-1976. Possibly a whole revolution. 00 13.0 +02 57 A 2001 1927-1944 too close. Apparent motion in a highly- inclined orbit. 00 13.2 +15 11 BUP 3 Gamma Peg. Beta CMa variable and spectroscopic binary. 00 13.2 +05 36 PLQ 3 Possibly same star as HDO 5 (Doolittle). 00 13.2 -17 11 HJ 1944 B is BD-17@16. Proper motion of B -062 -007. 00 13.4 +26 59 STT 2 P = 368yr., a = 0.56", motion retrograde. C is physical. 00 13.7 +49 34 STF 9 B is BD+48@42. 00 13.8 +36 12 BU 1341 AB: Proper motion of B +021 -026. AC: This is a measure of A and BD+35@27. Proper motion of BD+35@27 -012 000. 00 13.9 +63 23 BU 1309 AB: The star is 63@703-62@1909 in Vat. Astrog. Cat. (Van Biesbroeck). AD: D is 63@656-62@1910. 00 14.1 +76 01 STT 1 B is BD+75@5. Proper motion of B +002 -007. 00 14.5 -07 47 BU 486 Irregular variable, AD Cet. 00 14.8 +62 50 STF 10 Proper motion of B +020 -001. 00 15.0 +08 49 STF 12 35 Psc. A is an Algol-type system, UU Psc, P = 0.84d. Proper motion of B +106 -033. 00 15.2 +27 17 KUI 2 A is a spectroscopic binary. 00 15.3 -40 06 WG 2 B is CPD-40@14. 00 15.3 -42 30 RST 3344 Proper motion of B +046 -002. 00 15.5 -16 08 HEI 299 L722-22. Astrometric binary now resolved. P = 4.9yr, a = 0.30, motion retrograde. 00 15.9 -05 36 STF 15 Proper motion of B +036 -020. 00 16.0 +48 35 HJ 1009 Proper motion of B -004 -014. 00 16.2 +76 57 STF 13 A premature orbit has been calculated. 00 16.2 +19 03 J 217 Measures scattered. 00 16.4 +43 36 HJ 1947 Proper motion of B +056 +007. 00 16.7 +36 29 STT 4 P = 115yr., a = 0.36", motion retrograde. 00 17.1 +38 41 CHR 123 Theta And. 00 17.2 -19 21 LDS 9 B is BD-20@34. 00 17.4 +35 50 WEI 1 Proper motion of B -050 -066. 00 17.4 +16 31 STF 20 Proper motion of B +050 +005. 00 17.4 +08 53 A 1803 Too close 1932, 1946-47, 1965-72. Modern measures show a close approach about 1985. Ambiguous case, P = 18 or 36yr., a = 0.12 or 0.20". Motion retrograde. 00 17.4 +02 21 STF 21 Proper motion of B -020 +052. 00 17.5 +00 19 STF 23 Optical. 00 18.0 +09 31 AG 1 Proper motion of B -029 -067. 00 18.2 +72 57 A 803 P = 297yr., a = 0.36", motion direct. 00 18.4 +44 01 GRB 34 AB: Proper motion of A +2860 +390. Proper motion of B +2884 +410. Premature orbits have been calculated. A is a BY Dra-type variable, CQ And, and a spectroscopic binary. C is optical. 00 18.5 -27 57 HJ 1949 B is CD-28@75. Proper motion of B +060 -016. 00 18.7 +43 47 STT 5 26 And. 00 18.7 +25 45 HJ 1015 Proper motion of B -026 -052. 00 19.2 +59 42 KR 4 A is an irregular variable, V377 Cas. 00 19.4 -08 49 HJ 1953 Iota Cet. Variable? 00 19.6 -28 08 LDS 12 Proper motion -275 -1292. 00 19.7 +60 46 LDS 6088 Proper motion of B -172 +038. 00 19.8 +75 18 HJ 1950 Proper motion of B +028 +060. 00 20.0 +38 14 S 384 Proper motion of B +003 -003. 00 20.3 -32 46 B 1025 Considerable motion, but no measures for more than 30 years. 00 20.6 +12 19 BU 1015 P = 135yr., a = 0.35", motion direct. 00 21.0 +67 40 HJ 1018 STF 18. P = 163yr., a = 1.24", motion direct. 00 21.4 +67 00 STT 6 P = 240yr., a = 0.46", motion retrograde. C is physical. 00 21.5 -67 44 HJ 3361 CD-68@10. 00 21.7 +65 48 HU 1006 Proper motion of B +056 -147. 00 21.8 +66 28 STT 7 Proper motion of D -011 -008. 00 22.4 +13 29 STF 27 42 Psc. Optical. Proper motion of B -008 -024. 00 22.6 +50 33 KU 67 B is BD+49@62. 00 22.6 +21 40 HJ 1959 Proper motion of B -020 -050. 00 22.9 -12 13 BUP 6 9 Cet. 00 23.9 +29 30 STF 28 B is BD+28@55. The variable, double-lined spectro- scopic binary BD+28@49 may belong to the system. 00 24.0 +38 35 BUP 7 A is a Mira-type variable, R And. 00 24.2 -13 05 VOU 83 Less than 0.1" in 1954 (Van Biesbroeck). Single in 1958. Star confused with HU 4 (00246). 00 24.3 +52 01 HU 506 Single 1934, 1953. A premature orbit has been computed. A is a spectroscopic binary, P = 28d:. 00 24.7 -53 59 HJ 3364 B is CPD-54@89. Optical. 00 25.3 +32 30 STF 29 Proper motion of B +049 -014. 00 25.3 +20 36 J 3246 Single 1958 (Van Biesbroeck). 00 25.7 -50 50 HJ 3365 B is CD-51@102. 00 26.1 +34 48 HJ 622 Proper motion of B +006 -013. 00 26.8 +07 22 DOO 23 Doolittle calls this HDO 21, BDS 210. This seems to be a different pair. 00 26.9 -05 31 SCJ 1 B is BD-06@72. 00 26.9 -83 08 I 177 Spectrum of B is F. 00 27.1 -07 53 A 431 P = 54yr., a = 0.36", motion retrograde. 00 27.2 +49 59 STF 30 B is BD+49@89. 00 27.2 +07 10 HDO 20 Measure by Doolittle: 1908.91, 272.1@, 11.34", 11.7-12.5. Evidently another pair. 00 27.6 -31 57 HJ 3367 Proper motion of B +075 -023. C is optical. 00 27.7 -16 25 HJ 1968 Optical system. 00 28.3 +63 44 HU 1007 A premature orbit has been calculated. Motion direct. 00 28.4 -20 20 B 1909 Ambiguous case. P = 5.6 or 11.2yr., a = 0.12 or 0.21". Motion direct. 00 29.1 -07 42 MLR 2 Round 1954-58 with 82-inch. Speckle measures show rapid motion. 00 29.4 +30 36 SMA 5 Proper motion of B +031 +013. 00 30.0 -03 57 HJ 322 12 Cet. Optical. 00 30.1 +29 45 BU 1095 28 And. A is a Delta Scuti-type variable, GN And. 00 30.6 +49 19 OL 86 BD identification is doubtful. 00 30.7 +32 08 STT 11 Proper motion of B +038 -035. B is BD+31@66. 00 30.8 +16 02 STF 32 Proper motion of B +042 -026. 00 31.0 +55 39 ES 116 Proper motion of B -004 +013. 00 31.0 -10 05 HJ 1981 A-BC. A is physical. BU 1158 BC. P = 135yr., a = 0.38". Motion direct. 00 31.1 +56 48 ES 2 BDS 269 same star. Proper motion of B +028 -080. 00 31.2 -61 02 HJ 3372 CD-61@81. 00 31.3 -19 09 B 6 Too close 1937, 1938. Round 1958 and 1975 with large telescopes. Angle decreasing. 00 31.4 +33 35 HJ 5451 A is a spectroscopic binary. B is BD+32@81. 00 31.4 -48 48 RST 11 Lambda (1) Phe. A is a spectroscopic binary. 00 31.5 -11 16 HJ 1980 Proper motion of B +091 -005. 00 31.5 -62 57 B 7 Beta (1) Tuc. A is a spectroscopic binary. Proper motion of B +089 -048. LCL 119 Beta (1) and Beta (2) Tuc. I 260 Beta (2) Tuc. P = 44yr., a = 0.38", motion retrograde. 00 31.8 +54 31 STT 12 Lambda Cas. A premature orbit has been computed. 00 32.0 +28 31 S 386 Proper motion of B -008 -025. 00 32.1 +67 15 VYS 2 ADS 433, MLB 377. The primary is an astrometric binary P = 16yr. Proper motion +1.723 -0.242. A premature orbit has been computed for the visible pair. Also a flare star, V547 Cas. 00 32.1 -05 11 A 111 Ambiguous case, P = 10.8 or 21.3 yr., a = 0.17 or 0.19", motion retrograde. C is physical. 00 32.2 -75 15 HJ 3374 B is CPD-75@48. 00 32.4 +15 39 STF 37 Proper motion of B +006 -050. 00 32.4 +06 57 MCA 1 51 Psc. A is a triple occultation system, and a resolved interferometer pair. B is BD+06@65. 00 32.6 +20 18 HJ 1982 52 Psc. 00 32.7 +78 07 STF 34 Proper motion of B +020 -062. 00 32.7 -63 02 B 8 Beta (3) Tuc. Common proper motion with Beta (1) and (2). 00 32.8 +28 17 STT 14 A is a spectroscopic binary. 00 33.3 +58 37 ES 1769 Proper motion of B +027 -012. 00 33.5 +40 06 HO 3 A premature orbit has been computed. 00 33.6 -26 06 HJ 3377 Proper motion of B 000 +015. 00 34.8 +42 53 HJ 1036 Proper motion of B +013 -003. 00 34.9 +26 27 COU 548 Originally entered as AG 4. 00 34.9 +18 54 S 387 Proper motion of B -001 -013. 00 35.2 +36 50 STF 40 Proper motion of B -037 -030. 00 35.2 -03 36 HO 212 13 Cet. P = 6.9yr., a = 0.24", motion direct. A is a spectroscopic binary, and may be a Delta Scuti-type variable. 00 35.5 +58 41 STF 38 Proper motion of B -005 -003. 00 36.0 +29 59 STF 42 A is a spectroscopic binary. 00 36.6 -49 08 LDS 21 A is a spectroscopic binary, P = 3.74d. B is CD-49@138. 00 36.9 +33 43 H 17 Pi And. H V 17. BDS 263, HJ 1030 identical. A is a spectroscopic binary, P = 143.6d. B is BD +32@102. 00 37.3 +58 01 BU 1097 Spectrum composite; A2+K. 00 37.3 -24 46 BU 395 Proper motion +1396 -014. P = 25yr., a = 0.67", motion direct. 00 37.4 -37 17 I 705 Many attempts, but only a few positive observations. 00 37.9 +03 00 HDO 30 Proper motion of B +017 -035. 00 38.4 +40 59 STF 44 Proper motion of B -017 -007. 00 38.4 +01 30 BAL 947 Probably ARG 47, BD+00@93. 00 38.7 +46 57 STF 45 Proper motion of B +016 +008. 00 38.8 +31 01 AG 430 B is BD+30@90. 00 38.8 -25 06 HJ 1991 B is CD-25@235. 00 38.9 -25 36 HJ 1992 B is CD-26@195. 00 39.3 +30 52 BU 491 Delta And. A is a long-period spectroscopic binary, P = 15000d (?). 00 39.6 +84 45 HJ 1986 B is BD+83@11. Proper motion of B +089 -021. 00 39.9 +21 26 STF 46 55 Psc. 00 40.0 +76 52 STT 5 B is BD+76@16. Proper motion of B +034 -001. 00 40.3 +43 43 HJ 1044 Proper motion of B -006 -016. 00 40.3 +24 03 STF 47 Proper motion of B +045 +009. 00 40.5 +56 32 BU 1349 Alpha Cas. H 18 AD: H V 18. Also HJ 1993. 00 40.5 -16 31 BU 109 B is BD-17@108. 00 40.7 -04 21 HJ 323 B is BD-05@100. Proper motion of B -003 -056. 00 41.3 +52 40 AG 299 Proper motion of B +053 +044. 00 41.6 +24 38 WRH Hynek 1. Not certainly resolved by Wilson in 1949, but successfully resolved by McAlister in 1980. 00 41.8 -56 30 HJ 3387 Xi Phe. Variable. 00 42.4 +04 10 STT 18 A premature orbit has been calculated. 00 42.6 -54 07 HJ 3388 B is CPD-54@159. Proper motion of B -068 -177. 00 42.7 -38 28 HDO 182 Lambda (1) Scl. 00 42.7 -65 37 I 440 Probable rapid motion, as yet undefined by the measures. 00 42.9 +20 47 A 2205 A premature orbit has been calculated. 00 43.4 -57 28 HJ 3391 Eta Phe. 00 43.5 +33 51 BUP 241 AB: B is BD+32@120. AC: Distances are 1321" and 1310". 00 44.5 -17 15 B 2513 Probably BD-18@118. 00 44.7 +48 17 BU 231 Omicron Cas. A spectroscopic binary, P = 1033:d. 00 45.3 +10 19 STF 58 B is BD+09@85. 00 45.7 +74 59 H 122 21 Cas. A is an Algol-type eclipsing and spectroscopic binary, YZ Cas, P = 4.47d. 00 46.2 -22 14 RST 4155 P = 48yr., a = 0.20". 00 46.4 +30 57 STF 1 B is BD+30@114. Proper motion of B -039 -027. 00 46.8 -52 00 HJ 3398 B is CPD-52@91. 00 47.3 +24 16 BUP 9 18 Cet. 00 47.4 +51 06 H 82 H V 82. B is BD+50@142. Proper motion of B +023 +003. 00 47.7 +12 53 STT 8 B is BD+12@90. Proper motion of B +086 -038. 00 47.9 -29 21 I 261 Rapid, but as yet undefined, motion. 00 48.4 +16 40 GCB 2 BD identification uncertain. 00 48.4 +05 17 BUP 10 Aa-B: Zeta And. A is an eclipsing and spectroscopic binary, P = 17.8d. The new visual pair, Aa, may be physical, but Aa-B is probably optical. Proper motion +758 -1146. 00 48.7 +18 41 BU 495 P = 162yr., a = 0.61", motion retrograde. 00 48.7 +07 35 BUP 11 Delta Psc. 00 49.0 +16 56 BUP 12 64 Psc. A is a spectroscopic binary, P = 13.8d. 00 49.1 +57 49 STF 60 Eta Cas. Proper motion of A +1141 -572. P = 480yr., a = 12.0", motion direct. A has been reported to be a spectroscopic binary, but this is not confirmed. 00 49.2 +57 20 A 921 A premature orbit has been computed. Motion direct. C is probably physical. 00 49.9 +30 27 STT 9 B is BD+29@139, proper motion +029 -024. 00 49.9 +27 43 STF 61 65 Psc. Proper motion of B +097 -022. 00 50.3 +35 48 STF 62 Proper motion of B -011 -010. 00 50.3 -34 29 HJ 3401 Proper motion of B +127 -028. 00 50.4 +50 38 BU 232 Orbits with P = 219, 179, 150yr., and a about 0.5" have been computed. Motion direct. 00 50.5 +75 38 HJ 1997 B is BD+74@31. Proper motion of B -001 -005. 00 50.7 +64 15 MCA 2 A spectroscopic binary and resolved interferometer pair. Composite spectrum: B9.5V+G0III-IV. Orbits with P = 11.4 and 12.2yr., a = 0.045 and 0.042", have been computed. Motion retrograde. 00 50.8 +32 03 A 922 No observations 1932-69. Apparently has completed nearly a revolution. 00 51.2 +22 11 KU 70 Proper motion of B -007 +004.n direct. 00 51.6 +22 37 A 1808 Orbits with periods around 110yr. and a ~0.13" have been computed. Motion direct. 00 52.1 -13 14 HU 201 P = 146yr., a = 0.60", motion direct. 00 52.4 -69 30 DUN 2 Lambda (1) Tuc. B is CPD-70@38. Proper motion of B +001 -075. 00 52.7 -24 00 BU 734 A is a spectroscopic binary. 00 53.0 -61 05 GLI 4 Proper motion of B +109 +020. 00 53.1 +61 07 BU 497 A is a spectroscopic binary. Otherwise, the system is optical. 00 53.3 +05 00 STF 71 Proper motion of B -007 +003. 00 53.3 +04 05 A 2307 P = 60yr., a = 0.24", motion direct. 00 53.5 +25 36 BRT 119 Pourteau 73 may be identical. 00 53.6 +68 35 AG 8 Proper motion of B +000 -022. 00 53.8 +54 34 ES 938 Proper motion of B +000 -004. 00 54.0 -25 03 HJ 3407 B is CD-25@344, spectrum F2V. Proper motion of B +036 -021. 00 54.3 +69 03 AG 9 Proper motion of B -058 -003. 00 54.6 +39 10 STF 72 B is BD+38@139. Proper motion of B +015 +004. 00 54.6 +19 11 STT 20 66 Psc. P = 360yr., a = 0.70", motion retrograde. 00 54.7 +08 34 WZ 2 Proper motion of B +012 +025. 00 54.8 -67 27 GLI 7 B is CPD-68@33. Proper motion of B -028 -003. 00 55.0 +58 58 BU 1098 Upsilon (1) Cas. 00 55.0 +23 38 STF 73 36 And. P = 168yr., a = 1.00", motion direct. 00 55.1 +13 33 STF 75 Proper motion of B +070 -084. 00 55.4 +46 11 ES 1298 The angle for 1914 has been increased 100 degrees. 00 55.8 -18 32 B 645 Probable rapid motion, but little observed. 00 56.6 -16 14 HJ 2002 Evidently a mistake in position angle by Herschel (HJ). 00 56.6 -56 33 LPO 1 Spectral type G5? 00 56.7 +60 43 BU 1028 Gamma Cas. A is a nova-like variable. 00 56.8 +60 22 BU 1099 P = 83yr., a = 0.25", motion direct. A is a spectro- scopic binary, P = 4.2d. There is also a 4.85y period, recently confirmed by speckle interferometry. 00 56.8 +38 30 HJ 1057 Mu And. 00 57.2 +23 25 FOX 116 Eta And. A is a spectroscopic binary, P = 115.7d. 00 57.3 +60 20 ARG 3 B is BD+59@149. Proper motion of B +001 +002. 00 58.1 +26 55 STF 77 Proper motion of B +008 +026. 00 58.2 -15 41 S 390 Proper motion of B +023 +013. 00 58.4 +54 26 HJ 2003 Proper motion of B -120 -066. 00 59.1 +05 23 STF 78 Proper motion of B -020 +014. 00 59.3 -00 40 A 1902 P = 86yr., a = 0.29", motion direct. 00 59.3 -56 52 LDS 6106 B is CD-57@396. 00 59.4 +00 47 STF 80 Proper motion of B +009 -012. B is BD+00@158. 00 59.6 -01 11 A 1903 P = 117yr., a = 0.33", motion direct. C is physical. 00 59.6 -75 49 GLI 8 B is CPD-76@82, spectrum G0/2V. 00 59.8 +06 29 KUI 4 The primary is variable, WW Psc. 01 00.1 +44 43 STF 79 Both A and B are spectroscopic binaries. Proper motion of B +009 -022. 01 00.3 +67 17 HJ 1061 Proper motion of B -002 +000. 01 01.0 +12 24 AG 11 Proper motion of B +030 -003. 01 01.2 -56 10 HJ 3412 B is CPD-56@199. 01 01.4 +11 55 BU 867 Misidentified in BDS and ADS. Corrections by Baize and Couteau. A premature orbit has been calculated. 01 02.3 +81 53 KNT 1 A is an Algol type eclipsing binary, U Cep, P =19.3d. There is circumstellar matter. B appears physical, proper motion +023 -002. 01 02.3 +05 52 A 2003 Close, 0.2" or under. Position angles show large changes. A premature orbit has been computed. 01 02.8 +02 14 A 2308 P = 62yr., a = 0.21", motion direct. 01 02.9 +41 21 HJ 1064 39 And. 01 03.0 +47 23 STT 21 P = 450yr., a = 0.82", motion direct. A may be a spectroscopic binary. 01 03.0 -04 50 BUP 13 25 Cet. 01 03.3 -60 06 HJ 3416 Spectrum F6/8III/IV. Proper motion of B -084 -113. 01 03.8 +22 32 J 874 J measures a pair 1912 - 1917: 345@, 3". 01 03.8 +01 22 STF 84 26 Cet. Proper motion of B +129 -025 BU 1355 AC: 1909 and 1921 measures disagree. BDS 494 same star. 01 04.0 +35 28 HO 213 A premature orbit has been calculated. 01 04.0 -64 09 B 1913 Spectrum composite: K0III/IV+A/F. 01 04.8 +01 35 A 2310 Single in 1948. Position angles vary widely. A premature orbit has been calculated. 01 04.9 +36 49 A 1515 Periods from 86 to 419yr. have been calculated. Possibly an ambiguous case. 01 05.1 +14 57 HJ 1068 72 Psc. A is a spectroscopic binary. 01 05.2 +26 14 HJ 1067 Proper motion of B +051 -008. 01 05.5 +21 07 AG 14 P = 145yr., a = 0.61", motion retrograde. 01 05.5 +15 23 STF 87 Proper motion of B +031 -135. 01 05.7 +21 28 STF 88 Psi (1) Psc. Proper motion of B +059 -017. 01 05.8 +04 55 STF 90 77 Psc. B is BD+04@176. Proper motion of B +020 -133. 01 05.8 -59 59 R 5 B is CPD-60@75. 01 06.1 -46 43 SLR 1 Beta Phe. Variable? 01 06.2 +32 11 S 393 Proper motion of B 000 -015. 01 06.5 +58 41 A 930 Motion direct. Round in 1989. 01 06.5 +01 54 HDO 42 Doolittle may have measured a different pair (see ADS). 01 07.2 +53 30 H 66 H IV 66. 01 07.2 +38 39 A 1516 P = 34yr., a = 0.16", motion direct. 01 07.3 -34 52 COO 6 Proper motion of B +030 +034. Optical pair. 01 07.8 -41 29 RST 3352 Upsilon Phe. P = 28yr., a = 0.21", motion direct. 01 08.1 +63 36 STI 184 The S component is an irregular variable, HS Cas. 01 08.3 +54 55 WCK Mu Cas. Proper motion of A +3424 -1596 (FK5). A is an astrometric and spectroscopic binary, now resolved. 01 08.4 +05 39 BUP 15 80 Psc. B is BD+04@192. 01 08.4 -55 15 RST 1205 Zeta Phe. A is an Algol-type system, spectrum com- posite, P = 1.67d. Both B and C are probably physical. 01 08.6 -10 11 BUP 16 Eta Cet. B is BD-10@239. 01 09.4 -56 36 HU 1342 P = 80yr., a = 0.27", motion retrograde. 01 09.5 +47 15 STT 515 Phi And. P = 372yr., a = 0.45", motion retrograde. 01 09.7 +35 37 BAR 1 Beta And. B,C and D are optical. 01 10.1 +51 45 STT 23 Proper motion of B -076 -027. 01 10.7 +80 21 STF 89 B is BD+79@32. Proper motion of B -058 -034. 01 11.1 +55 09 STT Theta Cas. A is a spectroscopic binary, B is optical. 01 11.2 +41 13 A 655 P = 172yr., a = 0.31", motion direct. 01 11.2 +37 43 HO 215 45 And. Single 1903, 1906 (Doolittle), 1907 (Aitken). The measure 1925.60, 117.8@, 155.5", 6. - 6 (Schembor), may be erroneous. Duplicity of A is questionable. 01 12.2 +51 32 STF 97 Proper motion of B +026 +004. 01 12.2 +48 00 HJ 2024 Probably identical with BU 236, BDS 633. 01 12.7 +53 11 HJ 2025 Proper motion of B +007 -016. 01 12.8 +37 00 COU 1058 Proper motion of B -023 -017. 01 12.9 +32 05 STF 98 B is BD+31@196a. The primary is a double-lined spectro- scopic binary, P = 2.21d. B may also be a spectro- scopic pair (Hube, Pub. Astron. Soc. Pacific 93, 490; 1981). Proper motion of B +005 -007. 01 13.0 +30 04 STT 26 A is a spectroscopic binary. 01 13.1 +29 42 A 1260 Angle increasing, with a probable close approach about 1950. 01 13.7 +24 35 STF 99 Phi Psc. A is a spectroscopic binary. 01 13.7 +07 35 STF 100 Zeta Psc. Both A and B are spectroscopic and occulta- tion binaries, B has P = 9.08d. BU 1029 BC: Single 1914 - 1951. 01 13.7 -50 40 HJ 3421 Proper motion of B +158 -082. B is CD-51@312. 01 14.4 -07 55 STF 3 37 Cet. B is BD-08@215. Proper motion of B +132 +272. 01 14.8 +60 56 BU 1100 Ambiguous case; P = 75 or 150yr., a = 0.36 or 0.58", motion retrograde. In addition, one component is a spectroscopic binary, P = 5.33d. 01 14.8 -00 58 BUP 18 38 Cet. 01 15.1 -45 32 BLM Nu Phe. 01 15.8 +09 47 A 2102 Quadrant change. Not seen 1948 - 1954. 01 15.8 -68 53 HJ 3423 Kappa Tuc. A premature orbit has been computed. I 27 CD; P = 86yr., a = 1.12", motion direct. 01 16.6 -02 30 BU 1358 39 Cet. A semiregular variable, AY Cet, and spectro- scopic binary, P = 56.8d. Radio flares and soft X-rays are observed, and a white-dwarf companion is revealed by IUE observations. 01 17.2 +68 10 HJ 1075 Proper motion of B -024 -011. 01 17.5 +21 05 STF 107 Proper motion of B -055 -035. 01 17.6 +48 59 ES 1208 Proper motion of B +007 -004. 01 17.6 +40 18 A 1521 Rapid change, but the measures are inadequate to define the motion. 01 17.8 +49 45 HU 520 Quadrant indeterminate. 01 18.5 +73 23 A 814 Not separated about 1951 (Van Biesbroeck). Possible quadrant change. 01 18.8 +37 24 STF 108 The A component is a spectroscopic binary. 01 18.8 -56 37 RST 29 Spectral type G5? 01 19.2 +58 21 STI 1560 B is BD+57@248. 01 19.6 -05 20 A 313 P = 116yr., a = 0.26", motion retrograde. 01 19.8 -00 31 STF 113 42 Cet. FIN 337 BC: P = 27yr., a = 0.13", motion direct. 01 20.1 +58 14 H 23 H III 23. Phi Cas. A is a spectroscopic binary. A quintuple system. C has spectral type B5/6Ia/be. 01 20.3 +13 46 AG 16 Proper motion of B +017 -023. 01 20.3 -48 41 HJ 3428 B is CD-49@378. 01 20.8 +11 27 AG 17 B is BD+10@167. Proper motion of B +096 -072. 01 20.8 +10 35 PLQ 13 B is BD+09@153. Proper motion of B +011 +049. 01 21.1 +64 39 S 397 35 Cas. B is BD+63@175. Proper motion of B -010 -013. 01 21.1 +15 40 J 227 B is variable (Couteau). 01 21.1 +07 36 SLE 257 The primary is a W UMa system, AQ Psc. 01 21.3 +11 32 BU 4 P = 180yr., a = 0.36", motion retrograde. 01 21.8 -24 08 SEE 13 Motion direct. A premature orbit has been computed. 01 22.0 -69 43 I 263 A premature orbit has been computed. Motion direct. 01 22.7 +17 12 STT 16 Proper motion of B -010 -011. 01 23.4 +58 09 STF 115 P = 210yr., a = 0.80", motion retrograde. 01 23.7 -62 17 RST 31 Spectral type G0? 01 24.0 -08 00 HJ 1079 44 Cet. A is a Delta Scuti-type variable, AV Cet. AB is optical. 01 24.0 -08 11 BU 505 Theta Cet. Optical pair. 01 24.3 -06 55 BU 1163 P = 16.11yr., a = 0.197", motion retrograde. The system is also detected as a spectroscopic binary. 01 24.5 +39 02 STT 17 B is BD+38@256. Proper motion of B -010 -002. D is BD+38@253. 01 24.6 +53 11 ES 2583 B is BD+52@332. 01 25.1 +45 37 A 939 P = 109yr., a = 0.18", motion direct. 01 25.2 -79 54 HJ 3443 B is CPD-80@23. 01 25.3 -59 30 HJ 3435 B is CPD-60@111. Proper motion of B +072 +014. 01 25.8 +60 14 BUP 19 Delta Cas. A spectroscopic and (perhaps) eclipsing binary. 01 25.9 +68 08 BU 1101 Psi Cas. C and D are optical companions of A. CD is physical. H 83 H V 83, SHJ 18. C is BD+67@124. 01 25.9 -47 54 RST 33 P = 189yr., a = 1.10", motion retrograde. 01 26.2 -67 51 DON 17 P = 345yr., a = 1.02", motion direct. 01 27.0 -00 09 STF 125 Proper motion of B -017 +003. 01 27.0 -32 33 LDS 2199 Some unconfirmed early observations. A is the semi- regular variable R Scl. 01 27.4 -22 20 RST 2261 CD-22@503. 01 27.7 +45 24 BU 999 Omega And. 01 27.7 +05 21 BU 1164 P = 64yr., a = 0.31", motion retrograde. 01 28.3 +14 29 AG 18 B is BD+13@217. 01 28.4 +07 58 S 398 B is BD+07@214. Proper motion of B +114 -011. 01 29.1 +21 43 HO 9 BC: The radial velocities of B and C differ by 30km/sec. Either the pair is optical, or one component is a spectroscopic binary (Griffen). 01 29.5 +30 54 BUP 20 B is BD+30@229. Proper motion of B +036 -003. 01 29.6 -21 38 SEE 14 48 Cet. 01 29.7 +22 50 A 1910 P = 70.7yr., a = 0.190", motion retrograde. C is probably optical. 01 29.9 +31 00 ENG 6 B is BD+30@232. 01 29.9 +14 13 AG 19 Proper motion of B 000 -043. 01 30.1 +41 31 HJ 1081 Proper motion of B -001 -009. 01 30.2 +06 09 STH Mu Psc. 01 30.3 +12 39 STF 129 Proper motion of B +011 -007. 01 30.5 -42 42 I 1609 This is the variable SY Phe. 01 31.5 +15 21 BU 506 Eta Psc. A is a Beta CMi-type variable. 01 31.6 -19 01 HJ 2052 B is BD-19@263. Proper motion of B +031 -007. BDS 796, HJ 3373 same star. 01 32.1 +16 57 STF 132 A is a spectroscopic binary, P = 36.6d. All visual companions appear to be optical. 01 32.1 +16 57 STF 132 A is a spectroscopic binary, P = 36.6d. All visual companions appear to be optical. Proper motion of B 000 -005. 01 32.3 -26 33 ARG 4 B is CD-27@523. 01 32.6 +54 45 ES 2584 Proper motion of B +015 -025. 01 32.7 -01 39 FIL 2 B is BD-02@235. Proper motion of B -034 +017. 01 33.1 +54 16 ES 2585 Proper motion of B +002 -002. 01 33.2 +60 41 STF 131 Spectrum of B: B3IV. 01 33.5 +60 39 BUP 22 B is BD+59@273. Proper motion of B -001 +016. 01 33.7 -12 13 HWE 4 P = 145yr., a = 0.92", motion retrograde. 01 34.5 +34 40 A 1913 AB: P = 111yr., a = 0.29", motion retrograde. 01 34.8 +69 54 STF 130 Proper motion of B -015 +033. 01 34.8 +29 35 BRT 5 An Algol-type system, RS Tri. Proper motion of B +015 -017. 01 34.9 +12 34 STF 136 Proper motion of B -001 -015. 01 34.9 -69 09 GLI 12 B is CPD-69@74. Proper motion of B -036 -003. 01 35.0 -29 55 DAW 31 AB: P = 4.6yr., a = 0.17", motion direct. BU 1000 AB-C: P = 113yr., a = 1.42", motion direct. 01 35.2 +83 21 STF 118 Optical. Proper motion of B +066 -035. 01 35.4 +63 05 MLB 280 Also classified K1V. 01 35.4 +41 23 ES 1494 Probably identical with ADS 1241 ( = ALD). 01 35.5 +31 18 STF 137 Proper motion of B +035 +008. 01 35.6 +61 17 STI 237 This and STI 239 are members of the multiple system HJ 1083. 01 36.0 +07 39 STF 138 Proper motion of B +019 -047. D is BD+06@245. 01 36.1 -29 54 HJ 3447 Tau Scl. A premature orbit has been computed. 01 36.1 -37 18 HJ 3448 Spectral type of A may be K. B is CD-37@605. 01 36.4 +79 09 STF 127 B is BD+78@50. Proper motion of B +014 -007. 01 36.8 +41 24 BUP 23 Upsilon And. A is a spectroscopic binary. Proper motion of B +016 +014. 01 37.4 +58 38 STT 33 Proper motion of B +017 +008. 01 37.4 -82 17 GLI 14 Spectrum G5III:+K1/2. 01 37.6 +22 33 STT 20 B is BD+21@218. Proper motion of B +131 -001. 01 37.6 +07 09 PLQ 19 Proper motion of B +076 -076. 01 37.6 -09 24 KUI 7 P = 29.05yr., a = 0.318", motion retrograde. 01 38.5 +73 02 HJ 2054 40 Cas. 01 38.6 -41 13 CPO 110 B is CD-41@445. 01 38.8 -17 58 LDS 838 LUY 726-8. UV Ceti,(flare binary). Both components are active flare stars. P = 26.5yr., a = 1.95", motion retrograde. 01 39.3 +52 57 STF 139 Proper motion of B +002 -013. 01 39.7 +46 02 EGB 1 ES 553. Proper motion of B -004 -016. 01 39.7 -37 28 HJ 3452 B is CD-38@572. Proper motion of B +009 -016. 01 39.8 -56 12 DUN 5 P = 484yr., a = 7.8", motion retrograde. 01 39.9 +15 15 STF 142 Probably optical. B is BD+14@251. Proper motion of B +220 -063. 01 40.6 +40 35 BU 1362 Tau And. A is a spectroscopic binary. Variable? 01 40.9 +49 52 HU 531 P = 98yr., a = 0.26", motion retrograde. 01 40.9 +11 17 A 2320 P = 37yr., a = 0.18", motion direct. 01 40.9 +01 38 A 2404 1928 - 1941 too close for good measures. Quadrant uncertain. 01 41.1 +18 17 A 2321 Minimum separation in 1930, 125@, 0.8". May be optical. 01 41.3 +25 45 STF 145 A is a spectroscopic binary, P = 4.43d. 01 41.3 +10 07 STF 146 B is BD+09@203. 01 41.4 -79 09 HJ 3467 Tau (1) Hyi. 01 41.7 +53 23 A 1268 Single in 1954-1958 with 82-inch. Few measures. 01 41.8 +42 37 MCY 1 An astrometric binary now resolved by infrared speckle interferometry. P = 19.5yr, a = 0.13". 01 42.3 +58 38 HJ 1088 Proper motion of B +006 +001. 01 42.4 -06 45 A 1 A premature orbit has been computed. 01 42.5 +20 16 HJ 2071 107 Psc. AC: Obviously optical. 01 43.2 +60 56 MLR 106 AB, AC same coordinates as STI 270. 01 43.3 +60 33 BU 1103 44 Cas. A is a spectroscopic binary. 01 43.3 -17 36 HJ 3455 B is BD-18@292. Proper motion of B +038 +017. 01 43.4 -07 05 STF 150 B is BD-07@283. Proper motion of B +003 -010. 01 43.5 +53 18 HJ 2069 B is BD+52@417. 01 43.7 +09 34 BU 509 P = 233yr., a = 0.85", motion retrograde. 01 43.8 +12 06 HJ 18 Possibly BD+11@225. BDS 899, HJ 18. HJ position angle in 1820: 220@. Disagrees with 1912 - 1922: 143@. 01 44.1 -15 56 BUP 25 Tau Ceti. Optical. Proper motion of A -1718 +856. 01 44.3 +66 52 HAU Proper motion of B +131 -055. 01 44.3 +57 32 BU 870 A premature orbit has been computed. 01 44.3 +09 29 STF 155 Proper motion of B +110 -088. 01 44.8 +57 08 B 2548 Rapid motion. 01 45.0 +57 07 BU 453 Premature orbits have been calculated. Motion direct. 01 45.0 +43 42 STF 154 Proper motion of B +007 -023. 01 45.0 +27 03 COU 750 Rapid motion. 01 45.5 -60 35 JSP 13 JSP 13a. 01 45.6 -25 03 HJ 3461 Epsilon Scl. A premature orbit has been computed. 01 45.9 +71 42 HJ 1089 Proper motion of B -008 -014. 01 45.9 -43 57 HJ 3463 B is CD-44@509. 01 46.2 +33 43 HU 804 A premature orbit has been computed. 01 47.7 +63 51 ENG 7 B is BD+63@241. 01 47.7 -43 58 I 52 P = 252yr., a = 0.46", motion retrograde. 01 47.8 -80 11 HJ 3474 Tau (2) Hyi. 01 48.7 +61 50 HJ 1091 Proper motion of B -009 -007. 01 48.7 -29 16 HJ 3466 B is CD-29@590. 01 48.8 -01 25 STF 171 B is BD-02@300. 01 49.2 +34 04 STF 164 Proper motion of B -006 -029. 01 49.3 +47 54 CHR 4 B is a spectroscopic binary. The system appears to be quintuple. 01 49.6 -10 41 ENG 8 Proper motion of B -129 -087. 01 49.7 -10 22 BU 1168 Distance was very small and position angles uncertain after 1929. Round 1957. Now opening. 01 49.7 -14 14 HU 422 P = 99yr., a = 0.26", motion retrograde. 01 49.9 +80 53 STT 34 Orbits with P = 173 and 410yr., a = 0.38 and 1.30", motion direct and retrograde, have been computed. Obviously premature! 01 50.0 +27 06 STF 172 Proper motion of B -016 -011. 01 50.1 +22 17 STF 174 1 Ari. Spectrum composite; K1III+A6V. Spectroscopic binary? 01 51.0 +21 07 STF 175 Proper motion of B +098 +067. 01 51.2 +24 39 HO 311 P = 119yr., a = 0.30", motion direct. 01 51.3 +64 51 STF 163 B is BD+64@244. Proper motion of B +012 -015. 01 51.4 +43 29 HJ 2089 B is BD+42@388. Proper motion of B +016 -010. 01 51.5 -10 20 BNU Zeta Cet. A is a long-period spectroscopic binary, P = 1652d, and has been resolved by speckle interferometry. B is BD-11@360, proper motion +077 -013. AB optical. 01 51.7 +45 49 ARG 51 Proper motion of B +008 -008. 01 52.3 -09 44 BU 259 Proper motion of B -018 -025. 01 52.7 +57 17 ARG 6 Proper motion of B -005 +004. 01 52.8 -04 47 RST 4188 P = 263yr., a = 0.48", motion direct. 01 53.1 +29 35 BUP 27 Alpha Tri. A is a spectroscopic binary, P = 1.77d. 01 53.2 +37 19 STF 179 Proper motion of B +004 -072. 01 53.3 +40 44 HJ 1094 55 And. 01 53.4 +70 03 STF 169 Proper motion of B +023 -004. 01 53.5 +19 18 STF 180 Gamma Ari. A is a variable of the Alpha CVn type. Proper motion of B +077 -115. 01 54.1 -77 29 JSP 31 Apparent rapid retrograde motion, but measures sparse. 01 55.1 +28 47 STF 183 P = 368yr., a = 0.54", motion retrograde. C is physical. 01 55.3 -21 34 DON 26 CD-22@641. 01 55.4 +02 57 A 2407 A premature orbit has been computed. 01 55.9 +01 51 STF 186 P = 165yr., a = 1.02", motion direct. Spectroscopic binary? Spectrum composite; F7V+G0V. 01 56.0 +00 46 RST 5186 BD+00@311a. 01 56.0 -51 37 HJ 3473 Chi Eri. 01 56.1 +60 35 AG 301 Proper motion of B +077 -054. 01 56.1 +15 07 AG 26 Proper motion of B -017 +002. 01 56.2 +37 15 BU 1368 Bb: b is BD+36@349. STF 4 56 And. B is BD+36@354. 01 57.0 +31 01 A 819 A premature orbit has been computed. 01 57.2 +26 18 HJ 3243 Proper motion of B +044 000. 01 57.9 +23 36 H 12 H V 12. Lambda Ari. A is a Beta Lyrae-type and spectroscopic binary. B is BD+22@289. 01 58.0 -02 04 BU 7 Proper motion of B +040 +005. 01 58.1 +41 23 S 404 Proper motion of B -006 +009. 01 58.3 -82 18 I 311 Composite spectrum: G8/K0(V)+(G). 01 58.8 -22 12 HJ 2103 B is BD-22@329. Proper motion of B 000 +018. 01 58.9 -56 52 LDS 63 B is CPD-57@385. Proper motion of B +139 +131. 01 59.0 -22 55 H 58 H II 58. A is a W UMa-type system, AA Cet. 01 59.4 +50 36 AG 302 Proper motion of B +012 +010. 01 59.5 +62 54 STF 188 Proper motion of B -007 -003. 02 00.2 +06 41 STF 198 Proper motion of B +002 -015. 02 00.3 -01 38 BAL 9 Proper motion of B -002 -038. 02 00.4 -08 31 HJ 3476 A is AR Cet, probably a semi-regular variable. 02 00.5 -62 46 HJ 3479 B is CPD-63@142. Proper motion of B +041 +008. 02 00.6 +27 53 J 3257 A is an Algol-type binary, X Tri, P = 0.97d. 02 00.9 -43 50 I 265 After a close approach in the 1970's, the pair is opening up. 02 01.1 +35 18 STF 197 Proper motion of B -011 -001. Optical pair. 02 02.0 +70 54 BU 513 48 Cas. P = 60yr., a = 0.65", motion direct. A is a spectroscopic binary, same period as the visual pair. C is physical. 02 02.0 +02 46 STF 202 Alpha Psc. Both components are variables of the Alpha CVn type. Proper motion of B +033 -030. A premature orbit has been computed. A may be a spectroscopic pair. 02 02.2 +36 43 A 1813 AB: P = 12.9yr., a = 0.12", motion direct. AB-C: P = 330yr., a = 1.13", motion retrograde. 02 02.6 +07 41 HJ 647 Proper motion of B -007 -013. 02 02.7 -30 19 HJ 3478 B is CD-30@717. Proper motion of B -007 -020. 02 02.9 +11 22 STF 206 Proper motion of B +022 -010. 02 03.0 +33 17 STF 201 Epsilon Tri. Proper motion of B -011 -018. 02 03.1 -07 25 STF 209 B is BD-08@371. Proper motion of B +078 +019. 02 03.2 +55 14 BLL 4 A is a semi-regular variable, XX Per. B is BD+54@445. 02 03.7 +25 56 STF 208 10 Ari. P = 325yr., a = 1.39", motion direct. 02 03.8 -00 20 H 102 H V 102. 61 Cet. Spectrum composite; G5II-III+G5V. 02 03.9 +82 21 HJ 2090 The measure in BDS by COG belongs to some other pair. 1904.69, 243.9@, 3.52" (VBS). 02 03.9 +42 20 STF 205 H III 5, SHJ 26. Gamma And. STT 38 BC: P = 61yr., a = -.30", motion retrograde. B is a spectroscopic binary. 02 04.2 +52 57 HJ 2104 B is BD+52@501. Proper motion of B -023 +001. 02 05.1 +77 17 SHJ 22 47 Cas. 02 05.4 -09 47 J 1450 Proper motion of B +155 -009. 02 05.4 -59 10 HJ 3481 B is CPD-59@185. 02 05.5 +76 07 BU 785 49 Cas. 02 05.7 -24 23 I 454 CPD-24@891. C is CPD-24@889. 02 06.2 +25 07 STF 212 Proper motion of B -021 -033. 02 06.8 +25 42 HO 312 11 Ari. 02 07.4 -59 41 HJ 3484 B is CPD-60@183. 02 07.6 +15 35 STF 214 Proper motion of B +008 -010. 02 07.6 -00 37 LDS 3346 Proper motion of B -245 -363. 02 08.7 -00 26 STF 218 Proper motion of B -036 000. 02 09.1 +40 48 STF 215 A is an eclipsing binary, BX And. 02 09.4 +25 56 H 69 H VI 69. 14 Ari. Proper motion of B +065 -034. 02 09.7 +20 21 STF 221 Proper motion of B -007 +023. 02 09.9 +34 49 HU 1034 Not seen 1948, 1951. No observations since that time. 02 10.3 +33 22 STF 219 Proper motion of B +019 -005. 02 10.4 +39 11 HJ 1109 C is a nebula. 02 10.9 +39 02 STF 222 59 And. Proper motion of B -017 -013. 02 11.1 +12 20 AG 33 Proper motion of B +006 +030. 02 11.5 +57 39 BU 874 5 Per. 02 11.9 -72 41 GLI 16 Proper motion of B +034 +027. 02 12.2 +44 40 HJ 2117 A is a W UMa-type binary, GZ And. 02 12.4 +30 18 STF 227 Iota Tri. A is a spectroscopic binary, P = 14.73d. B is also a spectroscopic binary, P = 2.24d. One component is variable: TZ Tri. 02 12.4 -70 23 R 15 B is CPD-70@131. 02 12.8 +79 41 S 405 A is a Delta Scuti-type variable and spectroscopic binary, P = 4.12d. B is BD+78@71. 02 12.8 -02 24 STF 231 66 Cet. B is BD-03@335. Proper motion of B +366 -073. 02 12.9 +57 12 STT 24 Proper motion of B +145 +001. 02 13.0 +08 51 MCA 5 Xi (1) Cet. Also a spectroscopic binary. 02 13.2 +44 14 CHR 5 60 And. A spectroscopic binary. 02 13.5 -25 46 HJ 2120 B is CD-26@800. 02 13.6 +51 04 BAG 6 Per. A is a long-period spectroscopic binary, now resolved by speckle interferometry. 02 13.7 -03 02 H 110 H VI 110. B is BD-03@341. 02 14.0 +47 29 STF 228 P = 144yr., a = 0.91", motion direct. 02 14.4 +34 54 HU 807 Motion in separation, with little angular change. Close 1950-1960. 02 14.5 +66 31 MCA 6 55 Cas. Spectrum composite; B9V+G0II-III. 02 14.7 +30 24 STF 232 Proper motion of B +023 +041. 02 14.9 +58 29 STF 230 Proper motion of B -033 +002, spectrum B9IV. 02 15.7 +67 40 ENG 10 B is BD+66@193. Proper motion of B -018 -006. 02 15.7 +25 03 COU 79 21 Ari. P = 23.70yr., a = 0.235", motion retrograde. 02 15.7 +10 46 STF 237 Proper motion of B +064 -071. 02 15.8 -18 14 HTG 1 P = 173yr., a = 2.01", motion direct. 02 15.9 +06 38 A 2013 Ambiguous case, P = 73 or 35yr., a = 0.47 or 0.36", motion retrograde. 02 16.2 -23 02 I 457 ADS 1744a. 02 16.5 -51 31 DUN 6 Phi Eri. B is CPD-52@284. Optical pair. 02 16.9 +57 03 STT 25 B is BD+56@470. Proper motion of B +034 -011. 02 17.1 +34 13 DOR 66 Delta Tri. A is a double-lined spectroscopic binary, P = 10.02d. Proper motion +1154 -247. 02 17.4 +61 21 STF 234 P = 144yr., a = 0.54", motion retrograde. 02 17.4 +28 45 STF 239 Proper motion of B +093 -081. 02 17.6 +22 14 STF 244 Proper motion of B -042 -043. 02 18.1 +57 31 BU 1170 7 Per. 02 18.2 +39 20 A 207 P = 157yr., a = 0.30", motion direct. 02 18.6 +40 17 EGG 2 Proper motion of B -063 -015. 02 18.7 +04 12 BU 437 Proper motion of B -052 -048. 02 19.0 +28 39 HJ 1115 10 Tri. 02 19.3 -02 59 JOY 1 Omicron Ceti. Prototype of the Mira-type variables. "Orbits" have been computed for the visual pair, but are most likely false. All distant companions are optical. B is a Cepheid, VZ Cet. H 1 H VI 1. C is BD-03@355. 02 19.7 +60 02 STT 26 Proper motion of B -005 -008. 02 19.8 -23 52 HJ 2130 B is CD-24@1022. 02 19.8 -35 27 HJ 3494 P = 352yr., a = 1.85", motion retrograde. 02 20.0 -22 13 BRT 1373 CD-22@784. 02 20.2 +29 49 A 961 P = 180yr., a = 0.38", motion retrograde. 02 20.9 -56 32 RST 51 CD-57@470. 02 21.1 +42 46 STF 248 P = 300yr., a = 0.91", motion retrograde. 02 21.2 +56 51 BU 1171 Not seen in 1951 with 82-inch (Van Biesbroeck). 02 21.2 +21 36 HU 425 P = 125yr., a = 0.36", motion retrograde. 02 21.3 -10 57 HJ 3495 B is BD-11@445. 02 21.6 +23 38 STF 254 Proper motion of B +019 +002. POU 178. 02 22.4 +55 51 BU 875 9 Per. Variable, V474 Per. 02 22.9 +58 35 BLL 7 A is the semi-regular variable, S Per. Proper motion of B +009 -030. 02 23.1 +70 21 MLR 377 A premature orbit has been published. 02 23.2 -29 52 BU 738 P = 305yr., a = 1.40", motion retrograde. 02 23.3 +15 25 AG 38 B is BD+14@387. 02 23.5 +26 23 KU 76 Proper motion of B -016 -008. 02 23.6 +74 06 STF 241 Proper motion of B -005 +003. 02 23.9 +55 22 BU 1373 The primary is the variable V440 Per. 02 23.9 +33 30 STF 258 Proper motion of D -036 -012. 02 24.5 -01 45 STF 265 Proper motion of B +068 +047. 02 24.9 -02 07 STF 266 Proper motion of B +001 -015. 02 24.9 +51 53 ES 764 B is BD+51@567. 02 25.6 +50 17 BUP 31 65 And. 02 25.7 +61 33 STF 257 P = 580yr., a = 0.68", motion direct. One component is a spectroscopic and eclipsing pair, V559 Cas, P = 1.58d. 02 25.7 -21 19 HJ 3500 Proper motion of B +033 +038. 02 26.0 -15 20 H 80 H III 80. A is a variable of the Alpha CVn type, AB Cet, and a spectroscopic binary. 02 26.5 +54 17 STF 260 Proper motion of B -058 -027. 02 26.7 +32 07 A 964 Round 1951-1989. 02 26.8 +10 34 STT 27 B is BD+09@322. Proper motion of B +031 -030. A is VW Ari, a Delta Scuti-type variable. 02 27.7 +71 47 HJ 1116 Proper motion of B -010 +010. 02 27.8 +04 26 A 2329 P = 25.2yr., a = 0.55", motion direct. 02 28.2 +85 11 HJ 2110 Proper motion of B +029 -012. 02 28.2 +54 23 STF 267 B is BD+53@530. Proper motion of B +039 -004. 02 28.6 +55 21 ES 872 There is a difference of 18 degrees in the measured angles. The Espin measure appears correct. 02 28.8 +32 15 WOR 2 P = 23yr., a = 0.32", motion direct. 02 29.1 +67 24 STF 262 Iota Cas. A is a variable of the Alpha CVn type, and an astrometric and spectroscopic binary. A premature orbit has been computed for AB. Motion retrograde. A was detected as an astrometric binary, with P = 52yr., now resolved by speckle. 02 29.1 +23 31 VBS 6 Round 1953 - 1961. The inclination must be high. 02 29.2 +53 52 HJ 2136 Proper motion of B -003 -010. 02 29.4 +55 32 STF 268 A is a spectrum variable and shell star. 02 29.6 +60 39 STF 263 A is a possible Beta CMa-type variable, V528 Cas. C is a Beta Lyrae-type variable, V529 Cas. 02 29.6 +60 39 STF 264 A - A'. A - B'. A' is BD+60@486. Proper motion of A' -026 -020. 02 30.4 -30 21 HJ 3504 Proper motion of B +060 -019. 02 30.5 +05 04 PLQ 31 Proper motion of B -021 -025. 02 30.8 +55 33 STF 270 Proper motion of B +075 -095. 02 31.5 +01 06 STF 274 Proper motion of B -024 -023. 02 31.8 +89 16 STF 93 Alpha Umi. Polaris. A Cepheid variable and a spectro- scopic binary, P = 30yr. A close companion has been suspected. 02 31.9 +57 42 BU 1314 V425 Per. Variable in light and radial velocity. 02 32.0 +34 52 PTT 6 Proper motion of B +026 -010. 02 32.0 +18 22 STF 273 Proper motion of B -020 -011. 02 32.6 +09 35 HJ 652 Proper motion of B +108 +027. 02 32.7 +03 44 A 2334 Round 1953 - 1957. 02 33.0 +48 52 HJ 2144 B is BD+48@694. Proper motion of B -001 -002. 02 33.2 -22 07 DON 35 CD-22@863. 02 33.3 +52 19 STT 42 Distance small, measures often discordant. P = 136yr., a = 0.14", motion direct. 02 33.3 +00 08 GAU 1 Proper motion of B -009 -009. 02 33.5 +57 32 HJ 2143 B is BD+56@657. Proper motion of B -001 +007. 02 33.8 -28 14 HJ 3506 Omega For. 02 34.4 -42 59 HJ 3510 Spectrum: G3/5III/IV. 02 34.7 -07 52 BUP 32 77 Cet. 02 35.3 +40 17 A 1818 Round 1951-1960. Baize suspected another close pair in the region. 02 35.8 +34 41 AG 304 15 Tri. B is BD+34@471. Proper motion of B +002 -010. 02 35.9 +05 36 STF 281 Nu Cet. 02 36.0 -07 50 BUP 33 80 Cet. 02 36.1 +06 53 PLQ 32 Proper motion of A +1811 +1451 (FK5). Spectroscopic binary. 02 36.3 -63 29 B 1435 Spectral type F6? 02 36.6 +12 27 MCA 7 31 Ari. P = 3.9yr., a = 0.08", motion retrograde. 02 37.0 +24 39 STF 5 30 Ari. A is a spectroscopic binary. B is BD+24@375. Proper motion of B +142 -018. 02 37.0 +12 17 PLQ 33 Proper motion of B -023 +001. 02 37.1 +05 44 PLQ 34 Proper motion of B -024 +027. 02 37.1 -11 12 HU 1216 P = 162yr., a = 0.50", motion direct. 02 37.9 +20 03 A 2219 P = 98yr., a = 0.19", motion retrograde. 02 38.2 +46 04 A 1278 A premature orbit has been computed. 02 38.2 +29 08 BRT 7 A-BC is 340 degrees, 68". A is BD+28@445. (Heintz) 02 38.6 +03 27 KUI 9 HR 775 in Cetus. Some scatter in measured position angles. 02 38.7 -52 57 COO 14 Spectrum: F8IV/V + G/K. 02 38.9 -54 50 HJ 3520 B is CPD-55@444. 02 39.0 +62 35 STT 28 B is BD+61@445. Proper motion of B +035 -028. 02 39.0 +14 52 STF 287 Proper motion of B +036 -022. 02 39.0 +08 55 STT 30 Proper motion of B -013 -007. 02 39.1 +28 54 KU 77 Proper motion of B +017 +002. 02 39.2 +03 43 A 2336 Proper motion of B +007 -033. 02 39.3 -01 54 STF 290 Proper motion of B +073 +003. 02 39.6 -11 52 FIN 312 Epsilon Cet. P = 2.7yr., a = 0.11", motion direct. 02 39.9 +00 09 A 1928 P = 17.7yr., a = 0.14", motion direct. 02 40.2 +07 53 AG 45 Proper motion of B +001 -041. 02 40.7 +61 17 STF 284 A is a Beta CMa-type variable, V482 Cas. Proper motion of B +014 +012. 02 40.7 +27 04 STF 289 33 Ari. A spectroscopic binary. Proper motion of B +052 -044. 02 40.7 +26 37 STT 43 P = 475yr., a = 1.21", motion retrograde. 02 40.8 +15 00 AG 47 Proper motion of B +002 -005. 02 41.0 +65 39 STF 282 Proper motion of B +118 -062. 02 41.0 +34 50 AG 44 Proper motion of B -016 -013. 02 41.2 -00 42 STF 295 84 Cet. A is a Delta Scuti-type variable. 02 41.5 +40 53 COU 1511 P = 19.7yr., a = 0.12", motion retrograde. 02 41.5 +40 15 AG 46 Proper motion of B +021 +005. 02 42.0 +42 48 HJ 1123 B is BD+42@588, spectrum B9IVp(Hg,Mn,Eu). 02 42.2 +40 12 MCA 8 12 Per. Double-lined spectroscopic binary resolved by speckle interferometry. 02 42.4 +20 01 BLA Mu Ari. P = 8.8yr., a = 0.05", motion direct. 02 42.5 +40 16 STF 292 B is BD+39@611. Proper motion of B +023 -012. 02 42.7 +76 49 HJ 2146 Proper motion of B -003 -002. 02 42.8 +42 49 HJ 2155 B is BD+42@605. 02 42.8 +37 09 STF 294 Proper motion of B -006 +006. 02 43.3 +03 14 STF 299 Gamma Cet. Proper motion of B -180 -121. 02 43.4 -66 43 FIN 333 Probably an ambiguous case, although only one solution has been tested: P = 28.5 yr., a = 0.28", i = 90@. 02 44.2 +49 14 STF 296 Theta Per. Proper motion of C +009 -011. A premature orbit has been computed. 02 44.2 -25 30 FIN 379 Aa. More than one revolution apparently has occurred. Proper motion of a +162 +046. 02 44.3 +57 04 STF 293 Proper motion of B +086 -014. Optical pair. 02 44.6 +29 28 STF 300 Proper motion of B -026 -009. 02 44.7 -01 58 STF 303 Proper motion of B -004 +006. 02 44.9 +10 07 TOK Mu Ceti. Considered somewhat uncertain by Tokovinen. Not resolved by McAlister on several occasions. 02 45.2 -67 00 GLI 18 Spectrum: F5/6III/IV. 02 45.4 +56 34 MLR 599 Proper motion of B +013 -010. 02 45.5 -63 42 HDO 306 Gamma Hor. A spectroscopic binary. 02 46.0 -04 57 BU 83 A premature orbit has been calculated. 02 47.0 +47 05 AG 50 Proper motion of B +015 -014. 02 47.0 -09 52 A 2608 Proper motion of B +043 -002. The northern pair, CD, is slightly fainter (Heintz). 02 47.0 -13 20 RST 3371 Variable: CU Eri. 02 47.3 +17 17 A 2222 Proper motion of C +003 -004. 02 47.5 +19 22 STF 305 Proper motion of B +098 -145. A premature orbit has been computed. 02 47.6 +53 57 STF 301 A is a long-period spectroscopic binary, P = 675d. Proper motion of B +008 -016. 02 47.7 +05 51 STF 309 Proper motion of B +018 -011. 02 48.0 +07 34 AG 52 Proper motion of B +016 -034. 02 48.6 -37 24 HJ 3532 Proper motion of B +101 +024. 02 48.9 +38 23 ALD 10 First measure probably 90@ in error. 02 49.1 -32 24 B 1031 Beta For. 02 49.3 +17 28 STF 311 Pi Ari. A is a spectroscopic and occultation binary. 02 49.5 +57 05 MCA 9 V480 Per. 02 49.7 +12 09 AG 54 Proper motion of B -006 +007. 02 49.8 -20 15 HJ 3533 B is BD-20@523. Proper motion of B +037 -032. 02 49.8 -24 34 BU 877 Gamma (1) For. 02 49.9 +08 56 STF 313 Proper motion of B +048 -009. 02 50.0 +27 16 MCA 10 41 Ari. Aa is a spectroscopic binary and resolved interferometer pair. H 116 Aa-C: H V 116. H 5 Aa-D: H VI 5. D is BD+26@470. 02 50.2 -35 51 HJ 3536 Eta (2) For. 02 50.6 +38 19 BUP 34 16 Per. 02 50.7 +55 54 STF 307 Eta Per. A is a spectroscopic binary. B is BD+55@712. Proper motion of B +016 -012. 02 50.9 +03 31 PLQ 36 Proper motion of B +211 -039. 02 51.0 -21 00 SEE 20 Tau (2) Eri. 02 51.1 +60 25 STF 306 Spectroscopic binary, also classified Oe5V and O7.5. AC: See BDS 1430. 02 51.2 +60 23 D 28 See BDS 1431. 02 51.3 +03 03 HO 218 Position angle and distance changing rapidly but period not established. Needs speckle. 02 51.6 +60 33 BU 1374 Proper motion of B -001 -002. 02 51.7 +45 59 A 1281 P = 172yr., a = 0.55", motion direct. 02 51.7 -52 34 HU 1562 P = 65yr., a = 0.28", motion retrograde. 02 51.8 +58 19 BLL 8 A is a spectroscopic binary. B is BD+57@652. 02 52.0 -53 47 BRT 2020 CD-54@578. 02 52.1 +37 18 STF 316 Proper motion of B -011 -005. 02 52.1 -60 54 HJ 3540 CD-61@515. 02 52.9 +10 40 AG 56 Proper motion of B +036 -014. 02 53.5 +12 19 AG 57 Proper motion of B -004 -026. 02 53.7 +38 20 BU 524 AB: 20 Per. P = 31.4yr., a = 0.26", motion retrograde. A is a suspected variable. STF 318 AB-C: C is physical. Proper motion of C +033 -086. 02 54.3 +52 46 LAB Tau Per. Spectrum composite; G4III+A4V. A is a long- period spectroscopic binary, resolved by speckle interferometry. The 52" distant double companion may be physical. 02 54.4 +09 46 HJ 658 Proper motion of B +016 +002. 02 54.8 +43 32 HJ 2162 Star C is A of HJ 2163, BDS 1479. 02 55.6 +13 11 HU 1047 Close, position angles scattered. No positive observations since 1937. 02 55.8 +34 29 STF 325 Proper motion of B +124 -100. 02 55.8 +19 09 A 2342 Closing in with little angular change. 02 56.3 +58 52 STF 321 B is BD+58@531. Proper motion of B +011 +004. 02 56.5 +55 26 LDS 5401 Duplicity first noted by Ross: Ross 364-5. 02 56.7 +42 48 LDS 6141 A is possibly the same as A of LDS2815. 02 57.2 +01 53 A 2413 P = 114yr., a = 0.60", motion direct. 02 57.2 -00 34 STF 330 Proper motion of B -018 -015. 02 57.2 -24 58 BU 741 P = 137yr., a = 1.55", motion direct. 02 57.5 +14 20 AG 59 Proper motion of B +017 -010. 02 57.8 +44 31 STF 328 Proper motion of B +121 -017. 02 57.9 +00 25 STF 332 Proper motion of B +068 +024. 02 58.0 +21 24 J 233 Proper motion of B +013 +012. 02 58.1 +69 12 STF 317 BDS mentions a third star 15 sec f at 102.4@. 02 58.3 -40 18 PZ 2 Theta Eri. A is a spectroscopic binary. Proper motion of B -017 -006. 02 58.4 -01 35 A 208 C is BD-02@528. 02 58.6 +24 08 BU 1173 P = 440yr., a = 0.34", motion direct. C is probably physical. 02 58.8 +43 22 LDS 2816 B is BD+42@664. 02 58.9 +21 37 BU 525 Orbital solutions with P = 240 or 450 yrs., a = 0.44 or 0.57", motion direct, have been computed. 02 59.2 +21 20 STF 333 Epsilon Ari. Variable velocity suspected. 02 59.6 -25 16 LDS 3446 Zeta For. 03 00.1 +39 11 ALI 765 A is the eclipsing binary ST Per. 03 00.3 +14 32 AG 60 Proper motion of B +009 -019. 03 00.3 -11 18 A 2611 Too close 1940-1945 for good measures. Single 1948, 1954-1955. P = 68yr., a = 0.22", motion direct. 03 00.6 +47 53 A 1529 Round 1951 - 1954. 03 00.7 +57 00 KR 15 Heintz gives the correct identification and position. 03 00.9 +59 40 STT 31 B is BD+59@581. Proper motion of B +005 -022. 03 00.9 +52 21 STF 331 Both components are spectroscopic binaries. Proper motion of B +014 -005. 03 01.0 +65 24 STI 418 Proper motion of B +009 -014. 03 01.1 +44 53 HJ 2167 Proper motion of B +038 -034. 03 01.2 +59 02 STF 329 Proper motion of B +003 -015. 03 01.7 +02 33 BAL 1629 Proper motion of B +014 -033. 03 01.8 +58 51 MLB 53 Proper motion of B -010 +002. 03 01.8 +10 51 STF 338 Proper motion of B +034 -029. 03 02.0 +03 48 HDO 62 Proper motion of B +006 +001. 03 02.3 +18 20 A 2414 A premature orbit has been computed. 03 02.3 -71 54 FIN 360 Theta Hyi. Not seen for certain 1962-1969, and not observed since. Needs speckle. 03 02.7 -07 41 BU 11 Rho (2) Eri. 03 03.6 +36 27 BUP 37 Proper motion of B +018 -003. The Couteau companion, a, was suspected by Burnham. 03 04.6 -51 19 DUN 10 B is CD-51@706. Proper motion of B +096 +063. 03 04.7 +63 46 STF 335 B is BD+63@388. Proper motion of B -007 +006. 03 04.8 +53 30 WRH Gamma Per. Also a spectroscopic binary. Spectrum composite; G8III+A2V. Now resolved by speckle interferometry. B, at 57", is uncertainly physical. 03 04.9 +34 46 HU 812 HU position angle 1902: 199.4@. Probably wrong quadrant. 03 05.1 +70 12 HJ 1129 Proper motion of B -004 -029. 03 05.4 +25 15 STF 346 52 Ari. P = 227yr., a = 0.47", motion direct. 03 06.1 +79 25 STF 320 Spectroscopic binary? Spectrum composite; M1III+F7IV. 03 06.3 +51 00 AG 305 Proper motion of B +026 -032. 03 07.5 -78 59 HJ 3568 A is a spectroscopic binary. Proper motion of B +084 +069. 03 07.6 +75 48 HJ 2166 Proper motion of B -004 -013. 03 07.7 +36 37 ENG 11 B is BD+36@631. Proper motion of B 000 -011. 03 08.1 +24 35 STF 354 Proper motion of B +035 -018. 03 08.2 +40 57 LAB Beta Per. Algol, prototype of the Algol-type binaries. Also, a spectroscopic binary with P = 1.86 yr. 03 08.7 +17 36 COU 2680 BD+17@499a. 03 09.0 +44 15 STF 351 B is BD+43@637. 03 09.1 +49 37 BUP 38 Iota Per. Proper motion of A +1263 -091. 03 09.2 +07 28 STF 6 Proper motion of B -001 +008. B is BD+06@487. 03 09.5 +44 51 ES 2596 Kappa Per. A is a spectroscopic binary. 03 09.6 +05 12 A 2030 P = 55yr., a = 0.27", motion retrograde. 03 10.1 -63 55 HJ 3559 B is CPD-64@231. Proper motion of B +044 -012. 03 10.4 +02 38 OL 177 Position corrected by Heintz. 03 10.8 +63 47 STF 349 Proper motion of B +059 -052. 03 10.8 +15 08 GLP 1 Proper motion of B +004 +027. 03 11.2 +22 25 H 117 H V 117. 03 11.3 +39 37 BLL 10 Omega Per. 03 11.7 +81 28 STF 327 A is a spectroscopic binary. 03 12.1 +60 57 ES 1878 Proper motion of B +077 -217. 03 12.1 -28 59 HJ 3555 Alpha For. P = 314yr., a = 4.37", motion direct. B is probably variable. 03 12.1 -64 20 HJ 3562 B is CPD -64@231. Proper motion of B -026 -012. 03 12.2 +37 13 STF 360 A premature orbit has been calculated. 03 12.4 -44 25 JC 8 P = 45yr., a = 0.44", motion retrograde. HJ 3556 AB-C: C is in slow retrograde motion. 03 12.7 +71 33 STT 50 A premature orbit has been calculated. 03 12.8 -01 12 HJ 663 94 Cet. 03 13.6 +39 09 STF 364 Proper motion of B +058 -045. 03 14.0 +00 44 STF 367 P = 790yr., a = 1.31", motion retrograde. 03 14.3 +22 57 STF 366 Proper motion of B -010 -027. 03 14.6 +67 02 HJ 1132 Proper motion of B -011 +006. 03 15.2 -64 27 DUN 12 Proper motion of B -039 -063. 03 15.3 +44 51 KU 13 Proper motion of B -011 -002. 03 16.0 +34 41 HO 503 A spectroscopic binary and ellipsoidal variable, V423 Per. 03 16.3 +60 02 STF 362 Proper motion of B -026 +006. 03 17.1 +40 29 STF 369 Proper motion of B +045 -035. 03 17.2 -23 02 H 18 H N 18. 03 17.5 +65 40 STT 52 A premature orbit has been calculated. 03 17.7 +38 38 STT 53 P = 113yr., a = 0.50", motion retrograde. 03 17.8 -14 07 HU 432 Elongated, round or too close 1925-1937. 03 18.2 -62 30 BNU Zeta (2) Ret. B has common proper motion, +1370 +660, and is CPD-63@217, Zeta (1) Ret. 03 18.4 -00 56 AC 2 95 Cet. Orbit rather uncertain, solutions giving P = 352 or 217yr., a = 1.08 or 0.97", motion direct. Common proper motion with -01@474 at 11'. 03 18.4 -22 31 SEE 23 15 Eri. CD-22@1146. Motion direct. 03 18.7 -18 34 HJ 3565 A is a spectroscopic binary. 03 18.9 -01 01 BU 1177 P = 221yr., a = 0.45", motion retrograde. 03 19.2 -53 06 HJ 3571 CD-53@674. 03 19.4 +03 22 STT Kappa (1) Cet. Variable? A is a spectroscopic binary. B is BD+02@521. 03 19.5 -21 45 JC 1 Tau (4) Eri. A is an irregular variable. 03 20.0 +65 39 BUP 43 Shell star. Light and spectrum variable, BK Cam. May also be a long-period spectroscopic binary. 03 20.1 -28 51 LDS 93 BGH reports a third star at 38@, 105.6". B is CD-29@1229. 03 20.3 +19 44 STF 376 Proper motion of B +033 -009. 03 20.7 +84 59 STF 319 Schiller measures 1910.87,331.1@,42.32",7.7-9.2. 03 20.7 +46 41 BU 1294 Proper motion of B -006 -022. 03 20.7 +17 36 HJ 3245 See BDS for components. 03 21.1 +43 22 A 1705 Proper motion of B -020 -009. 03 21.2 +21 09 COU 259 Tau (1) Ari. A is an irregular variable. 03 21.2 +05 23 BAL 2995 Proper motion of B -043 -024. 03 21.7 +08 45 STF 380 A premature orbit has been calculated. 03 21.9 +49 04 WEB 1 B is BD+48@892. 03 22.1 +62 44 STF 373 Proper motion of B +023 -034. 03 22.9 +29 49 STF 379 H III 91, BDS 1688. Proper motion of B +028 -016. 03 23.2 +24 12 KU 80 Proper motion of B 000 -017. 03 23.3 -50 00 HJ 3573 A is CD-50@1015, B is CD-50@1014 (Roman). 03 23.6 +04 53 BU 1178 A is a spectroscopic binary. 03 24.0 -26 13 HJ 3572 B is CD-26@1270. Proper motion of B -048 +013. 03 24.2 +67 28 STF 374 Proper motion of B +000 -054. 03 24.2 +17 33 STF 383 Proper motion of B 000 -054. 03 24.3 +49 52 BUP 44 Alpha Per. 03 24.4 -15 39 A 2909 P = 25yr., a = 0.15", motion direct. There are many negative observations. Needs speckle. C may be physical. 03 24.5 +58 26 STF 378 Proper motion of B -005 -015. 03 24.7 +78 31 STF 363 Proper motion of B +008 -001. 03 25.4 -01 09 SCJ 2 Proper motion of B -035 -016. 03 26.1 +12 29 A 829 Probably ambiguous case, but only one solution has been tested: P = 121yr., a = 0.30", motion retrograde. 03 26.6 +28 43 CHR 9 UX Ari. 03 27.1 +18 45 CHR 10 Resolution of an occultation binary. 03 28.0 +20 28 STF 394 Proper motion of B -007 -019. 03 28.2 -35 51 I 58 Chi (3) For. 03 28.4 +60 15 A 980 P = 231yr., a = 0.38", motion retrograde. 03 28.4 +22 48 BAG 66 Ari. A is a spectroscopic and occultation binary, now resolved by Balega et al. 03 29.4 +49 31 BU 1179 34 Per. 03 29.4 -62 56 HJ 3580 Kappa Ret. 03 29.8 +50 01 ES 2599 Proper motion of B +016 +009. 03 30.0 +55 27 STF 390 Proper motion of B -032 +019. 03 30.8 +05 09 STF 406 Proper motion of B -025 -016. 03 31.0 +29 37 A 983 P = 184yr., a = 0.35", motion direct. 03 31.1 +27 44 STF 7 B is BD+27@513. Proper motion of B +026 -034. 03 31.2 +19 47 STF 403 Proper motion of B -001 +008. 03 31.3 +27 34 STF 401 Proper motion of B +023 -041. 03 31.3 -59 55 JSP 47 CD-60@724. 03 31.6 +47 52 STT 56 Proper motion of B +020 +018. Optical pair. The primary also is classified B8.5VeShell. 03 32.0 +67 35 STT 54 B is BD+67@274. Proper motion of B +037 -042. 03 32.1 +43 40 COU 1688 A premature orbit has been calculated with very sparse data, since most of the observations are negative. 03 32.3 -07 05 STF 411 B is BD-07@619 (Roman). Proper motion of B -043 -049. 03 32.9 -09 27 BLA Epsilon Eri. 03 33.2 +04 09 AG 69 Proper motion of B -025 -024. 03 33.5 +58 46 STF 396 B is BD+58@618. Proper motion of B +023 -052. Spectrum of A: Am(A3/A7/F0). 03 33.9 -31 05 B 52 P = 19.13yr., a = 0.24", motion direct. 03 34.2 +48 37 BU 787 C does not exist (van den Bos). Optical pair. There is, nevertheless, a premature orbit. 03 34.4 +24 28 STF 412 7 Tau. P = 375yr., a = 0.56", motion retrograde. Spectrum composite; A3V+A3V. Star C is physical. 03 34.5 +19 48 STF 414 H III 78. Proper motion of B -011 +001. 03 35.0 +60 02 STF 400 P = 288yr., a = 1.24", motion direct. 03 35.0 +32 01 STF 410 A is an ellipsoidal variable, IX Per. 03 35.3 +26 51 STF 415 Proper motion of B +028 -033. 03 36.2 +42 20 A 1535 P = 153yr., a = 0.56", motion direct. 03 36.8 +00 35 STF 422 A premature orbit has been computed. The primary is a variable of the RS CVn type, V711 Tau., and also a spectroscopic binary. 03 37.4 -80 51 HJ 3607 B is CPD-81@89. Proper motion of B +010 -011. 03 37.8 +40 45 COU 1517 This is the variable AB Per. 03 38.2 -59 47 DUN 14 B is CPD-60@261. Common proper motion +025 +053. 03 38.3 +44 48 S 430 B is BD+44@759. Proper motion of B +030 -032. 03 39.6 +25 30 LDS 6158 This is the common proper motion pair Wolf 204,5. 03 40.0 +63 52 HU 1062 BC: Perhaps half a revolution. Round 1924 (Van Biesbroeck). Needs speckle. 03 40.3 -08 05 STF 433 B is BD-08@698. 03 40.5 +05 08 STF 430 Proper motion of B +004 -018. 03 40.6 +28 46 STF 427 Proper motion of B +059 -040. 03 40.7 +46 01 STT 59 Proper motion of B +010 +003. 03 40.7 +06 43 A 1934 Companion not seen in 1934. 03 40.9 -12 37 STF 436 B is BD-13@712. Proper motion of B +013 +018. 03 41.1 +60 39 ARG 57 B is BD+60@727. Proper motion of B +007 -019. 03 41.3 +45 54 BU 1181 Motion in separation. The period may be fairly short. Needs speckle. 03 41.8 +62 39 BLL 12 A is a semi-regular variable, U Cam. B is BD+62@594. 03 42.2 +54 36 HJ 2198 B is BD+54@704. Proper motion of B -013 -006. 03 42.3 +31 41 COU 691 A premature orbit has been computed. 03 42.4 +33 58 STF 431 40 Per. A spectroscopic binary. Spectrum of B: A1Vn. 03 42.4 -80 01 HJ 3612 Spectrum: G0/2III/IV. B is CPD-80@94. 03 42.5 +02 02 BAL 1260 Proper motion of B +075 -019. 03 42.8 +30 16 AG 72 Proper motion of B +015 -020. 03 42.9 +47 47 BUP 46 Delta Per. A possible variable of the Alpha CVn type. Proper motion of B -008 -005. 03 43.1 +25 41 STF 435 Proper motion of B -050 -010. 03 43.9 -71 00 HJ 3603 B is CPD-71@218. 03 44.0 +38 22 STF 434 B is BD+37@821. Proper motion of B +011 +005. 03 44.1 +32 07 STF 437 Proper motion of B +010 +005. 03 44.2 -64 48 LDS 104 Beta Ret. A is a spectroscopic binary. B has separation of 1480". B is CPD-65@272. 03 44.3 +32 17 BU 535 Omicron Per. Ellipsoidal and spectroscopic binary. 03 44.4 +28 12 A 1826 Not seen on three nights 1964-1982. 03 44.6 +27 54 STT 38 Optical with BU 1041BC, which is BD+27@558, at 03 44.7 +27 55. 03 44.6 -54 16 HJ 3592 See claimed A was a close pair in 1897, but no trace of it was seen subsequently by van den Bos, Dawson, and Innes. 03 45.2 +42 35 ES 2601 Nu Per. 03 45.2 +24 28 HJ 3251 19 Tau. A is a spectroscopic and occultation binary. Proper motion of B +026 -012. 03 45.4 -27 52 BU 1003 A premature orbit has been computed. Motion direct and increasing as the pair closes in. However, there are no measures in the last twenty years. 03 45.5 +66 06 AG 71 Proper motion of B +017 -004. 03 45.7 +06 03 HJ 2204 29 Tau. A is a spectroscopic binary. 03 45.7 -13 20 STF 451 Proper motion of B -009 -026. 03 45.8 +23 09 STF 444 Spectroscopic binary, P = 7.15d. 03 46.1 -64 05 HJ 3600 B is CPD-64@271. Proper motion of B +026 -005. 03 46.2 +71 37 STF 421 Proper motion of B +010 +025. 03 46.3 +24 11 BU 536 A premature orbit has been computed. Motion retrograde and rectilinear so far. 03 46.4 +75 23 PRZ 4 Proper motion of B 000 -001. 03 46.5 +24 15 CHR 12 Pleiad. 03 47.0 +41 26 STF 443 Proper motion of A +599 -1250. Proper motion of B +599 -1267. B is a single-lined spectroscopic binary, P = 48.65d. A common proper motion companion, G 95-59, mag. 13.4, lies more than 2 degrees away. 03 47.0 +24 31 CHR 124 Occultation binary. Has variable radial velocity. Pleiad. 03 47.1 +24 49 BU 537 Variable, V534 Tau. 03 47.4 +24 40 STF 449 Proper motion of B -011 -016. 03 47.5 +24 06 STF 8 Eta Tau. A is an occultation and spectroscopic binary. B, at 03 47.4 +24 07, is an occultation binary. C is V647 Tau. 03 47.9 +33 36 STF 448 HJ 5457. A is a spectroscopic binary. Also, one component is variable. 03 47.9 +25 55 BRT 2520 Heintz finds no pair in the field, and believes identity with J 27 (03470+2855) is possible. 03 48.0 +68 40 KUI 13 BC: P = 44yr., a = 0.44", motion retrograde. A is physical. 03 48.0 +38 21 STF 447 Proper motion of B -001 +001. 03 48.0 -70 48 HJ 3606 B is CPD-71@223. 03 48.1 +24 09 COU 80 Pleiad. 03 48.2 +24 19 CHR 155 Pleiad. 03 48.3 +11 09 STF 452 30 Tau. 03 48.4 +52 02 HU 546 P = 69yr., a = 0.32", motion retrograde. 03 48.5 +01 36 STF 456 Proper motion of B +031 000. 03 48.5 -31 47 HJ 3596 Proper motion of B -015 -019 03 48.6 -37 37 DUN 16 One component is a possible Beta Lyrae-type system. Proper motion of B +033 -082 03 48.9 +64 45 STT 62 P = 188yr., a = 0.38", motion direct. 03 49.2 +24 08 CHR 125 Pleione, 28 Tau. A shell star, BU Tau, and suspected long-period spectroscopic binary. Pleiad. 03 49.2 +24 03 STF 453 27 Tau. Single 1843-1937, 1953. Position angles scattered. Distances range from "single" to 0.6". Some question duplicity. A is a long-period spectro- scopic binary. 03 49.3 +57 07 S 436 B is BD+56@847. Proper motion of B +036 -024. 03 49.4 +52 14 ES 770 B is BD+51@781. 03 49.4 +24 23 STT 40 B is BD+23@560. Proper motion of B +022 -039. A is an occultation double. 03 49.5 +52 39 STF 446 Another classification: B0Ib. The primary is slightly variable, and the system is a member of the cluster NGC 1444.1. 03 49.6 +38 59 HU 1067 A RW Aur-type variable, XY Per. Both components may vary. 03 49.6 +18 17 STF 458 Proper motion of B -010 -038. 03 50.0 +23 51 STT 64 A is a spectroscopic binary, P = 16.72d, spectrum B9.5VpSiSrCr. A Pleiad. 03 50.1 +44 58 CHR 126 A spectroscopic binary. 03 50.3 +25 35 STT 65 P = 62yr., a = 0.43", motion direct. 03 50.4 +71 20 HJ 2200 Gamma Cam. 03 50.4 +34 40 ES 236 Proper motion of B -023 +082. 03 51.3 +26 21 A 1830 The few observations do not define the nature of the motion. 03 51.6 +00 20 STF 463 Proper motion of B +006 +001. 03 51.7 +70 30 HJ 1139 B is BD+70@263. Proper motion of B -005 -022. 03 52.0 +06 32 KUI 15 31 Tau. 03 52.6 -08 29 RST 4762 The few measures do not define the motion. 03 52.7 -05 22 HJ 338 30 Eri. 03 53.2 -02 00 STF 466 Proper motion of B -027 -026. 03 53.7 +53 16 A 1293 P = 57yr., a = 0.30", motion direct. 03 54.1 +31 53 STF 464 Zeta Per. A is a spectroscopic binary. 03 54.3 -02 57 STF 470 32 Eri. A is a spectroscopic binary. 03 54.4 -06 49 A 461 Less than 0.1" in 1954 - 1961. It appears that a revo- lution has been completed. 03 54.4 -40 21 FIN 344 Spectroscopic binary. 03 54.5 +05 10 STT 41 A is a Delta Scuti-type variable, V479 Tau. B is BD+04@600. A-BC is probably physical. A 1831 BC: Less than 0.1" in 1954 - 1955 with 82-inch. A premature orbit has been computed. Motion direct. 03 54.9 +21 48 OL 200 Possibly identical with HU 815 (03559+2147). 03 55.4 +31 03 HO 325 A is a RW Aur-type variable, X Per., and also a long-period spectroscopic binary. 03 55.7 -22 36 I 722 CD-22@1398. 03 56.6 +50 42 S 440 43 Per. A is a spectroscopic binary. B is BD+50@861. 03 57.1 +69 31 STF 455 Proper motion of B -015 -007. 03 57.1 -08 28 RST 4764 Rapid retrograde motion. 03 57.5 -01 10 BU 543 A premature orbit has been computed. A is a flare suspect. 03 57.8 +49 32 KU 82 B is BD+49@1068. 03 57.9 +40 01 STF 471 Epsilon Per. A is a Beta Lyrae-type binary. 03 58.0 -13 31 HJ 3608 Gamma Eri. Variable? 03 58.6 -02 39 BU 1042 B is BD-03@651. 03 59.6 +02 41 AG 76 Single in 1903 and 1910. Identification? 03 59.6 -10 19 HU 29 Too close 1937. Elongated 1938. 03 59.7 +48 09 STT 68 A is an Algol-type binary, IQ Per. B is BD+47@921. 03 59.8 +11 33 STF 478 Proper motion of B +044 -012. 03 59.8 +11 33 LDS 5464 Proper motion of B +036 -010. 04 00.8 +18 12 BUP 49 A is a spectroscopic binary. B is BD+17@664. 04 00.8 +08 38 PLQ 47 Proper motion of B +009 -002. 04 00.8 +05 05 A 1937 P = 44yr., a = 0.10", motion direct. 04 00.9 -10 27 STF 487 B is BD-10@814. 04 01.6 +38 40 STF 476 Proper motion of B -054 +016. 04 02.2 +28 08 STF 481 AD: Declination difference 11.18". 04 02.4 -28 32 DAW 79 P = 161yr., a = 0.50", motion retrograde. 04 02.6 +79 01 HU 1070 Proper motion of B +017 -042. 04 02.7 +54 28 AG 307 Proper motion of B +026 -023. 04 03.8 +37 58 ES 2085 A is V380 Per. 04 03.8 -44 29 LCL B is CD-44@1388. 04 03.9 +28 08 VBS 9 An Algol-type binary, RW Tau. 04 04.0 +39 32 L Nothing at this position (Heintz). 04 04.1 +39 31 STF 483 P = 440yr., a = 2.14", motion retrograde. 04 04.4 +24 06 MCA 13 36 Tau. A is an occultation binary, now resolved by speckle interferometry. 04 04.7 +22 05 STT 37 Tau. Proper motion of B +008 -067. 04 04.9 -35 50 HJ 3622 Proper motion of B +002 -110. 04 05.0 +37 05 KU 83 Proper motion of B +035 -040. 04 05.3 +22 01 CHR 158 39 Tau. Variable? B is optical. Proper motion of B +003 -020. 04 05.9 +34 38 ES 238 A measure in 1946 gives distance as 7.2". 04 06.4 +43 25 A 1710 P = 110yr., a = 0.40", motion retrograde. 04 06.5 +14 22 S 443 B is BD+13@643. Proper motion of B +005 -006. 04 06.6 -60 19 R 40 B is CPD-60@292. Spectral type of B may be G8. Proper motion of B +006 +043. 04 06.8 +50 35 HU 547 Variable of unknown type. 04 06.9 +33 27 STT 71 A is an Algol-type eclipsing binary, AG Per, P = 2.03d. 04 07.6 +38 04 STT 531 Premature orbits have been calculated. Motion retro- grade. Common proper motion with BD+37@882, 50 Per, 12' distant. The primary is V491 Per. 04 07.7 +15 10 STF 495 A is a Delta Scuti-type variable. 04 07.8 +62 20 STF 485 Proper motion of B -005 -016. Refer to ADS for descripti tions. B is a Beta Lyrae-type system, SZ Cam, P = 2.7d. 04 08.0 +43 11 AG 308 B is BD+42@897. Proper motion of B -011 -031. 04 08.5 +08 27 STF 497 Proper motion of B +031 -024. 04 08.9 +29 11 BU 1232 Orbit highly inclined. P = 60yr., a = 0.28", motion direct. 04 08.9 +23 06 STF 494 Proper motion of B +018 -008. 04 09.0 -51 53 HJ 3625 B is CPD-52@499. 04 09.1 +28 39 HO 326 Two solutions exist, with P = 187 or 207yr., a = 0.39 or 0.67", motion direct. 04 09.3 -07 56 A 469 P = 126yr., a = 0.26", motion direct. 04 09.4 +78 26 HJ 2211 Proper motion of B +031 -004. 04 09.5 -17 29 ENG 17 B is BD-17@806. Proper motion of B -015 +007. 04 09.6 -60 23 R 41 B is CPD-60@297. 04 09.6 -81 51 RST 2345 A semi-regular variable, U Men. 04 10.0 +80 42 STF 460 P = 415yr., a = 1.00", motion direct. 04 10.5 +60 09 STF 490 Proper motion of B +015 -018. 04 10.7 -04 52 A 2801 Ambiguous case; P = 20 or 40 yr., a = 0.14 or 0.20", motion direct. 04 12.0 -09 16 A 471 Motion increasing, but only three measures since 1933. 04 12.2 +00 44 STF 510 Proper motion of B -015 +040. 04 12.3 +69 08 HJ 1141 A 13.3 magnitude star is 20" preceding. 04 12.5 +35 38 HJ 341 ALI 59. BU gives 1880 position +35 25. 04 12.5 -36 09 HJ 3628 B is CD-36@1632. Proper motion of B +066 +005. 04 12.6 +76 14 STF 474 Proper motion of B +005 +017. 04 13.2 +50 32 CHR 15 Ross 29. 04 13.2 +22 58 HU 302 A premature orbit has been computed. 04 13.6 +07 43 A 1938 46 Tau. P = 7.18yr., a = 0.136", motion direct. 04 13.9 +09 16 BU 547 47 Tau. 04 14.2 -46 08 RST 2338 P = 18.6yr., a = 0.25", motion direct. 04 14.4 -10 15 STF 516 39 Eri. 04 14.4 -62 28 HJ 3638 Alpha Ret. Possible spectroscopic binary. 04 14.9 +48 25 STT 73 Mu Per. A is a Beta Lyrae-type system. H 20 H VI 20. SHJ 364. 04 15.2 +50 52 AG 309 B is BD+50@944. Proper motion of B +081 -056. 04 15.3 -07 39 STF 518 Omicron (2) Eri. Proper motion of A -2224 -3423. BC: P = 252yr., a = 6.94", motion retrograde. B is a white dwarf, and C is a flare star, DY Eri, and a strong X-ray source. Omicron (1) Eri at 83" is physical, and is a Delta Scuti star showing coronal X-ray emission. 04 15.5 +06 11 H 98 H VI 98. A is V774 Tau. B is a suspected variable, and is BD+05@613. Proper motion of B -097 -109. 04 15.8 +45 24 STF 512 Proper motion of B +144 -191. 04 15.8 +15 24 BUP 51 45 Tau. 04 15.9 +31 42 STT 77 P = 190yr., a = 0.55", motion direct. C is physical. 04 16.3 -60 57 GLE 1 Variable: TT Ret. A premature orbit has been computed. 04 16.5 -59 18 JSP 56 Epsilon Ret. 04 17.0 +19 41 HO 328 P = 63yr., a = 0.36", motion retrograde. 04 17.1 +64 08 STF 503 BD is probably BD+63@489a. Proper motion of B +010 -011. 04 17.3 +46 13 STT 44 B is BD+45@904. 04 17.7 -63 15 RMK 3 Theta Ret. 04 17.9 +58 47 STF 511 P = 343yr., a = 0.54", motion retrograde. 04 17.9 -33 48 I 270 Upsilon (4) Eri. Duplicity of AB doubtful. A is a spectroscopic binary, and possible variable. 04 18.2 +22 48 STF 520 P = 227yr., a = 0.50", motion direct. 04 18.3 +67 34 STF 504 Proper motion of B +002 +006. 04 18.4 +21 35 MCA 14 51 Tau. B is BD+21@619. In 1957 B was not seen (van den Bos). A is a long-period spectroscopic binary, resolved by speckle interferometry. P = 11.3yr., a = 0.13", motion retrograde. 04 18.9 +01 46 STT 49 B is BD+01@734. Proper motion of B +017 +003. 04 19.3 -44 16 HJ 3643 B is CD-44@1505. Proper motion of B +064 -035. 04 19.8 +15 38 BLM Gamma Tau. A spectroscopic binary resolved by speckle interferometry. 04 19.9 +31 45 J 934 Couteau corrects the position. Jonckheere in 1958 gives the 1950 position: 04 17.0 +31 43. 04 19.9 +16 31 STT 79 P = 89yr., a = 0.56", motion direct. 04 20.0 +14 02 BUP 53 57 Tau. A is a Delta Scuti-type variable, V483 Tau. 04 20.4 +34 34 BU 1382 54 Per. 04 20.4 +27 21 SHJ 40 Phi Tau. B is BD+26@712. Proper motion of B -008 -002. 04 20.6 +24 30 COU 704 Probably the A component of POU 442. 04 20.9 +70 23 STF 506 Proper motion of B -010 +022. 04 21.0 +50 15 S 445 B is BD+49@1161. 04 21.1 +55 32 STT 46 B is BD+55@869. Proper motion of B +024 -005. 04 21.5 -25 44 BU 744 P = 81yr., a = 0.48", motion direct. 04 21.6 +06 58 A 1835 Round 1951 - 1955. 04 21.8 +19 49 KNT 2 The variable U Tau. 04 22.0 +28 26 ISM RY Tau, a T-Tauri star. 04 22.1 +14 05 BUP 54 60 Tau. A is a specroscopic binary and variable, V775 Tau. 04 22.4 +51 49 AG 310 Proper motion of B +023 -044. 04 22.6 +25 38 STF 528 Chi Tau. Proper motion of B +032 +003. 04 22.7 +15 03 STT 82 P = 256yr., a = 1.18", motion retrograde. The primary is a spectroscopic binary, P = 4.00d. 04 22.9 +17 33 BUP 55 Delta (1) Tau. The primary is a long-period spectro- scopic and occultation binary. 04 23.3 +11 23 STF 535 A premature orbit has been computed. 04 23.3 -21 38 B 2571 CPD-21@545. 04 23.5 +20 59 CHR 16 An occultation binary, now resolved. 04 23.9 +09 28 HU 304 66 Tau. P = 55yr., a = 0.20", motion direct. 04 24.0 +24 18 STF 534 62 Tau. 04 24.1 +17 27 BUP 56 Delta (2) Tau. Optical. A is a spectroscopic binary. 04 24.4 +34 19 STF 533 Proper motion of B +012 -011. 04 24.6 +33 58 STT 81 56 Per. 04 24.7 +69 12 HJ 1142 Proper motion of B +017 -021. 04 24.9 -77 41 HJ 3673 Proper motion of B -078 -004. 04 25.2 -64 15 HJ 3656 B is CPD-64@333. 04 25.3 +22 15 STF 541 J 2722. This faint pair is between Kappa (1) and Kappa (2) Tau. 04 25.3 +22 15 STF 541 Kappa (2) Tau. 04 25.4 +22 18 STF 9 Kappa (1) Tau. A is an occultation binary. 04 25.4 +02 21 HJ 2230 Proper motion of B +012 -002. 04 25.5 +17 56 KUI 17 Delta (3) Tau. A is a spectroscopic binary and variable, V776 Tau. H 101 H VI 101. There is a wide faint pair noticed by John Herschel, 320@ Class VI. 04 25.6 +15 56 FIN 342 Possibly an ambiguous case. P = 12.4 or 6.3yr., a = 0.10" (in either case). 04 25.9 +60 15 STF 526 Proper motion of B -010 +011. 04 25.9 +18 52 BU 1185 P = 28yr., a = 0.25", motion retrograde. 04 26.0 +45 15 ES 567 B is BD+44@946. Proper motion of B -004 -002. 04 26.2 +35 44 HU 608 Possibly an ambiguous case, P = 217 or 857yr., a = 1.64 or 1.25", motion direct. 04 26.3 +34 43 HU 609 P = 83.3yr., a = 0.24", motion retrograde. 04 26.3 +22 49 BUP 58 Upsilon Tau. A is an occultation binary. 04 26.3 +15 37 BUP 59 71 Tau. A is a long-period spectroscopic binary, P = 5200d, and occultation pair. V777 Tau. 04 26.9 -24 05 BU 311 P = 176yr., a = 1.25", motion direct. 04 27.0 +19 07 STF 546 Proper motion of B +105 -150. 04 27.0 -72 38 B 2091 Composite spectrum: G8III+(A/F). 04 27.1 +18 12 STF 545 Proper motion of B +002 -014. 04 27.5 +11 13 BU 1186 A is variable. 04 27.5 -24 27 I 413 P = 200yr., a = 0.99", motion direct. 04 27.8 +10 01 STF 549 Proper motion of B -001 -002. 04 28.0 +21 37 BUP 60 A is a spectroscopic and occultation binary. 04 28.4 -65 43 HJ 3662 B is CPD-65@345. Proper motion of B -013 +016. 04 28.6 +19 11 BUP 61 Epsilon Tau. 04 28.6 +15 58 MCA 15 Theta (1) Tau. Physical companion to Theta (2) Tau. A spectroscopic, occultation, and interferometric binary. 04 28.7 +15 52 STF 10 Theta (2) Tau. B is BD+15@631. Proper motion of B +082 -026. A spectroscopic and occultation binary. Also, variable, probably of Delta Scuti type. 04 28.9 +30 22 STF 548 A is a spectroscopic binary. Proper motion of B +018 -005. 04 29.0 +16 10 HU 1080 P = 40yr., a = 0.42", motion retrograde. 04 29.4 -33 35 HJ 3652 Variable, CT Eri. 04 29.5 +17 52 BGH Variable, V921 Tau. B is +17@ 734. 04 30.1 +18 14 JOY 2 A RW Aur-type variable, UX Tau. 04 30.1 +15 38 STF 554 80 Tau. P = 180yr., a = 1.00", motion retrograde. A is a single-lined spectroscopic binary. 04 30.2 +05 18 STF 556 Proper motion of B +045 -015. 04 30.6 +16 12 LDS 2246 A is an occultation binary, and possibly variable. B is BD+15@640. 04 30.6 +15 42 BUP 62 81 Tau. B is BD+15@638. 04 30.6 +13 43 BUP 63 83 Tau. 04 30.7 -16 27 HJ 3653 B is BD-16@879. Proper motion of B +004 -007. 04 30.9 +59 02 STI 2051 A is an astrometric binary. C is a white dwarf, in slow retrograde motion about the mass-center. 04 31.1 +06 47 STT 84 Proper motion of B -066 -085. 04 31.4 +40 01 STF 552 Proper motion of B +010 -006. 04 31.4 -13 39 STF 560 B is BD-13@905. Proper motion of B -004 -025. 04 31.7 +15 38 WOR 16 The A component is a known Hyad. LDS 1174 The C component may or may not be a physical companion, possibly sharing CPM only as a member of the cluster. 04 31.9 +07 49 BRT 2596 Proper motion of B +009 -007. 04 31.9 -08 51 HJ 2234 B is BD-09@917. 04 32.0 +53 55 STF 550 1 Cam. A spectroscopic binary. Proper motion of B +003 -001. 04 32.2 +52 12 STF 551 Proper motion of B -002 -014. 04 32.4 +01 18 HDO 307 Not found by Heintz. Identical with BAL 1273? 04 32.6 -03 13 H 64 H VI 64. Probably a variable of Delta Scuti type, DZ Eri. B is BD-03@810. 04 32.7 +25 53 JOY 3 A RW Aur-type variable, UZ Tau. 04 33.3 +52 48 ES 2607 B is BD+52@844. Proper motion of B +005 -012. 04 33.4 +43 04 SHJ 44 57 Per. 04 33.5 +72 32 HJ 2228 A is a spectroscopic binary. 04 33.5 +18 01 STF 559 Proper motion of B +003 -036. 04 33.6 -62 49 HJ 3670 B is CPD-63@343. Proper motion of B -115 -015. 04 33.9 -06 44 BU 881 46 Eri. A is the variable EH Eri, P = 3.8d, small amplitude. 04 34.0 -55 03 B 2092 Alpha Dor. P = 12yr., a = 0.20", motion direct. 04 34.1 +53 01 ES 2608 Proper motion of B -006 +009. 04 34.4 +16 30 OL 107 The ES pair formerly listed at 04350+1631 is identical to this pair. (Heintz). 04 34.9 +39 08 HU 1082 P = 52yr., a = 0.36", motion direct. 04 34.9 -76 51 HJ 3691 B is CPD-77@176. Proper motion of B +001 +009. 04 35.2 -09 44 STF 570 B is BD-10@958. Proper motion of B +019 -020. 04 35.3 -00 29 BAL 660 Proper motion of B -016 +006. 04 35.7 +10 10 CHR 18 88 Tau. A is an Alpha CVn-type variable, and spectro- scopic binary, now resolved by speckle interferometry. B is BD+09@606, with proper motion +053 -048. 04 35.9 +16 31 BU 550 Alpha Tauri. A is an unclassified variable. 04 36.2 +09 13 STF 569 Proper motion of B -028 -015. 04 36.2 +08 14 A 1840 Possibly an ambiguous case, P = 278 or 115yr., a = 0.29 or 0.26", motion retrograde. C is probably physical. 04 36.3 +47 22 S 451 B is BD+47@1012. Proper motion of B +001 -016. 04 36.3 -03 21 BUP 64 Nu Eri. A is a Beta CMa-type variable. 04 36.4 +34 13 HU 610 P = 58yr., a = 0.18", motion direct. 04 36.7 +19 30 LDS 3597 The primary is a BY Draconis-type variable, V833 Tau. 04 36.8 -17 33 A 2915 P = 195yr., a = 0.25", motion direct. The high- exccentricity solution yields P = 83yr., a = 0.23". 04 36.8 -62 05 HJ 3679 A is a long-period variable, R Dor. 04 37.4 +00 34 STT 53 B is BD+00@801. Proper motion of B +018 +018. 04 37.4 -09 51 RST 3401 P = 71yr., a = 0.23", motion retrograde. 04 38.0 -13 02 STF 576 B is BD-13@938. Proper motion of B +021 -018. 04 38.2 +16 02 BUP 65 89 Tau. Optical. 04 38.2 +12 31 BUP 66 90 Tau. A is a spectroscopic binary. 04 38.2 -14 18 KUI 18 53 Eri. P = 77.4yr., a = 0.707", motion direct. 04 38.5 +26 56 STF 572 One component is a spectroscopic binary. 04 39.1 +07 52 BUP 67 B is BD+07@680. 04 39.3 +15 55 STF 11 Sigma (2) Tau. B is BD+15@665, Sigma (1) Tau. Proper motion of B +032 -052. B is a spectroscopic and occultation binary. A is a spectroscopic binary. 04 39.5 -45 07 I 1489 P = 31.5yr., a = 0.21", motion direct. 04 39.9 +53 05 BU 1043 3 Cam. A is an eclipsing binary of the W UMa-type. 04 40.0 +53 28 BU 1295 2 Cam. AB: P = 26.89yr., a = 0.177", motion retrograde. STF 566 AB-C: P = 425yr., a = 1.38", motion retrograde. 04 40.1 +03 19 STF 578 Proper motion of B +004 -012. 04 40.3 -58 57 HJ 3683 P = 240yr., a = 1.90", motion retrograde. 04 40.4 -19 40 STN 9 54 Eri. A semiregular variable, DM Eri. No very posi- tive observations as a visual double. Needs speckle. 04 40.4 -29 35 HJ 3677 Proper motion of B -054 -075. 04 40.6 -41 52 HDO 190 Alpha Cae. A is a Delta Scuti-type variable. 04 41.7 -61 13 HJ 3686 Proper motion of B +028 +009. 04 42.2 +58 45 ES 56 Proper motion of B +010 +010. 04 42.2 +37 31 STF 577 A premature orbit has been computed. Motion retrograde. 04 42.2 +22 57 MCA 16 Tau Tau. Hough suspected duplicity due to a slow occul- tation. Finally resolved by McAlister in 1980. A is also a short-period spectroscopic binary. 04 42.2 +02 59 A 2424 Position angles uncertain. Too close 1929,1934,1951, 1953, 1955. Ambiguous case, P = 24.5 or 49yr., a = 0.09 or 0.18", motion retrograde. 04 42.7 +06 30 AG 81 Proper motion of B +001 -022. 04 42.7 +04 50 STF 585 Proper motion of B -004 000. 04 43.0 +57 12 A 1014 P = 74yr., a = 0.26", motion direct. 04 43.3 +59 31 A 1013 P = 126yr., a = 0.29", motion direct. 04 43.3 -09 37 BU 1384 Proper motion of B +047 +043. 04 43.6 -08 48 STF 590 55 Eri. B is a Delta Scuti-type variable, DW Eri., BD-09@969. Spectral type F4IIIpSr. Both components are spectroscopic binaries. 04 44.1 +02 05 HL 1 This is a measure of HL 04441+0204 and A 3006 04440+0204 04 44.4 +11 09 BUP 68 A may be variable. 04 44.8 +05 17 STF 589 Proper motion of B -149 -050. 04 45.0 +57 18 MLB 59 Proper motion of B +002 -017. 04 45.4 -59 49 FIN 89 A is the Mira-type variable, T Dor. 04 45.5 -05 12 HJ 27 B is BD-05@1021. 04 45.5 -22 26 DON 77 CD-22@1801. 04 45.8 +07 08 HJ 682 Proper motion of B +008 -026. 04 45.9 +19 11 AG 311 B is BD+18@714. Proper motion of B -006 -003. 04 46.0 +11 42 BUP 69 A is possibly a spectroscopic binary. Optical system. 04 46.4 +42 21 COU 2031 P = 6.8yr., a = 0.087", motion direct. Needs speckle. 04 46.5 +71 28 HJ 2235 Proper motion of B +026 -053. 04 47.2 +20 27 KU 85 Proper motion of B +003 -017. 04 47.2 -17 15 ARG 11 B is BD-17@951, spectrum G2/3V. 04 47.5 +43 24 A 1544 P = 78yr., a = 0.17", motion retrograde. C is physical. 04 47.7 +34 46 HJ 349 Proper motion of B -004 -041. 04 47.8 +53 18 HU 612 P = 157yr., a = 0.40", motion direct. 04 48.0 +56 45 BU 1387 4 Cam. 04 48.0 +53 07 STF 586 Same position, and in field of, STF 587. 04 48.0 +53 07 STF 587 Proper motion of B -017 +007. 04 48.5 +10 56 HJ 684 Proper motion of B -009 -012. 04 48.6 +17 48 STF 598 Proper motion of B 000 -040. 04 49.1 +05 13 STT 55 B is BD+04@755. Proper motion of B -004 -013. 04 49.3 +32 35 CHR 19 A spectroscopic binary with P = 7.05d. 04 49.6 +02 12 A 2621 P = 226yr., a = 0.18", motion direct. 04 49.7 +15 54 HJ 3261 96 Tau. 04 49.8 +06 58 STT Pi (3) Ori. Obviously an optical pair. A spectroscopic binary and possibly a variable of Delta Scuti type. 04 50.1 +66 32 STF 584 Proper motion of B -017 -032. 04 50.2 -31 13 B 1474 P = 97yr., a = 0.27", circular orbit with direct motion. 04 50.3 +06 57 H 83 H V 83. Proper motion of B -009 -014. 04 50.4 +09 34 A 2039 Proper motion of B +008 -010. 04 50.5 +01 03 A 2622 Round 1951 with 82-inch. A premature orbit has been computed. 04 50.8 -40 13 I 1492 Variable, Y Cae. 04 50.9 -53 28 DUN 18 Iota Pic. Proper motion of B -062 +067. 04 51.1 +44 58 STF 599 Proper motion of B +005 -009. 04 51.2 +11 04 BU 883 P = 16.3yr., a = 0.20", motion direct. 04 51.2 -22 13 BRT 1378 CD-22@1851. 04 51.3 -68 04 FIN 362 Only one observation, with many negative results. Duplicity questionable. Needs speckle. 04 51.4 +57 11 LDS 5614 Proper motion of B -006 -043. 04 51.4 +18 50 BUP 70 97 Tau. A is a Delta Scuti-type variable, V480 Tau. B is BD+18@742. 04 51.5 -34 54 FIN 320 Appears to have completed a revolution if the quadrants are correct. Period about 40yr. 04 51.6 +04 23 BAL 2619 Proper motion of B +001 +008. 04 51.8 +30 47 JOY 4 A is the RW Aur-type variable, UY Aur. 04 51.8 +13 39 BU 552 P = 95yr., a = 0.73", motion direct. A is a spectroscopic binary of period 143d. 04 51.9 -60 58 JSP 62 CD-61@974. 04 52.6 +37 49 ES 2337 Proper motion of B -005 +010. 04 53.1 +25 29 STF 607 Proper motion of B +001 -020. 04 53.1 -01 17 S 457 B is BD-01@743. Proper motion of B +017 -003. 04 54.2 +49 35 STF 603 Proper motion of B 000 +006. 04 54.3 +07 22 STF 612 Proper motion of B +244 -211. 04 54.8 +11 26 MCA 17 6 Ori. 04 54.9 +10 09 ENG 19 Pi (1) Ori. B is BD+09@682. Proper motion of B +021 -020. 04 55.1 +55 16 BU 1187 5 Cam. 04 55.2 +00 58 BAL 976 Proper motion of B +005 -003. 04 55.2 -79 23 HJ 3733 B is CPD-79@163. 04 56.3 +52 06 HU 555 P = 72yr., a = 0.21", motion direct. C is physical. Proper motion of C +053 -069. 04 56.4 +13 31 BU 553 Omicron (2) Ori. 04 56.4 -05 10 SHJ 48 62 Eri. B is BD-05@1093. Proper motion of B -016 -002. 04 56.6 -66 29 DON 89 Variable. 04 57.3 +53 45 D 5 7 Cam. A premature orbit has been computed for AB. A is a spectroscopic binary. STF 610 AB-C: C may be physical. 04 57.6 -05 45 STF 624 B is BD-05@1103. 04 57.8 +48 01 HJ 2241 Proper motion of B +004 -011. 04 57.8 +23 57 BU 1045 99 Tau. 04 58.0 -22 48 I 473 CD-22@1917. 04 58.2 +25 03 BU 1390 98 Tau. A is a spectroscopic binary. 04 58.5 -27 49 RST 117 CPD-28@715. 04 59.0 +69 19 STF 602 Proper motion of B -007 +001. 04 59.0 +14 33 SHJ 49 B is BD+14@795. Probably same as BDS 2461, H V 57. 04 59.0 -16 23 BU 314 P = 54.8yr., a = 0.50", motion retrograde. 04 59.1 +63 22 HU 1090 P = 26yr., a = 0.23", motion retrograde. 04 59.3 +37 53 STF 616 Omega Aur. 04 59.6 +80 08 ARG 59 Proper motion of B +023 -013. 04 59.9 +53 27 A 1303 A premature orbit has been computed. 04 59.9 +27 20 STF 623 Proper motion of B +014 -034. 05 00.1 -62 17 B 1942 Composite spectrum: G5/8III + F/G. 05 00.3 +39 24 CHR 159 5 Aur. 05 00.4 +69 25 STF 606 B is BD+69@289. Proper motion of B -008 -007. 05 00.5 +05 06 STT 93 A premature orbit has been computed. 05 00.6 +03 37 STF 627 B is BD+03@736. Proper motion of B +007 -033. 05 00.7 +03 16 STF 628 Proper motion of B -012 -002. 05 00.8 +39 13 AG 83 Proper motion of B +012 -036. 05 01.3 +50 15 STF 619 Proper motion of B +008 -090. 05 01.7 +26 40 A 1844 P = 25yr., a = 0.22", motion direct. 05 01.7 +20 50 HU 445 P = 145yr., a = 0.45", motion direct. 05 01.8 +11 23 S 463 Proper motion of B -013 -015. 05 02.0 +43 49 BU 554 Epsilon Aur. A is a enigmatic supergiant eclipsing system. 05 02.3 -56 05 LDS 135 B is CPD-56@767. 05 02.4 +04 19 AG 85 Proper motion of B +010 +005. 05 02.4 -64 54 GLI 32 B is CPD-65@416. 05 02.5 -21 15 DON 91 P = 43yr., a = 1.40", motion direct. 05 02.7 +04 36 AG 87 Proper motion of B +018 -017. 05 02.7 -33 09 HJ 3718 B is CD-33@2076. Proper motion of B -009 -007. 05 02.8 +52 03 AG 312 Proper motion of B -001 -012. 05 02.8 -49 09 RST 120 Eta (1) Pic. 05 03.3 -17 22 B 2583 LPM 202. L 736-49. 05 03.4 +63 00 STF 617 Proper motion of B -022 -029. 05 03.4 +60 27 S 459 Beta Cam. Proper motion of B -018 -036. 05 03.5 +63 05 STF 618 C is BD+62@721 (STF 617). Proper motion of B +013 +312. 05 03.7 -02 32 J 307 Single 1951,1953,1957. Reality of BC is in doubt. 05 04.4 +62 37 HU 1094 Stein measure 1901.3, 289@, 4.2", 9.5-9.9. For this position Hussey finds no such pair. 05 04.4 -35 29 JC 9 Gamma (1) Cae. The secondary is variable (Inf. Bull. Var. Stars 2736, 1985). 05 04.7 +74 04 STT 89 P = 136yr., a = 0.42", motion direct; inclination nearly 90 degrees. 05 04.7 -20 17 WHC 2 CPD-20@742. 05 04.9 -10 31 A 2633 BD-10@1086, 24" p and 1.3' s is also double: 6", 8.6-13.5. 05 05.2 +50 02 SMA 46 Proper motion of B -018 +000. 05 05.3 +69 23 HJ 2244 B is BD+69@295. Proper motion of B +001 -009. 05 05.6 +23 04 STT 97 See long note in BDS. Single in 1889. Recovered in 1976 1976 by McAlister. 05 05.9 -13 55 A 3009 P = 169yr., a = 1.03", motion direct. 05 06.1 +58 58 STF 13 11 Cam. B is 12 Cam., BD+58@805, spectrum K0III, is a spectroscopic binary, P = 80.2d. 05 06.7 +51 36 BU 1046 9 Aur. A is a spectroscopic binary. H 35 AC: H VI 35. 05 06.8 -04 39 STF 642 66 Eri. A is a spectroscopic binary. 05 07.0 +33 25 STF 640 Proper motion of B +006 +000. 05 07.0 -39 39 HJ 3725 B is CD-39@1789. Proper motion of B +002 +001. 05 07.1 +59 20 A 1025 Single in 1959 and 1989 with 15 and 24-inch refractors. Needs speckle. 05 07.4 +18 39 A 3010 104 Tau. Ambiguous and uncertain orbits of P = 1.2 and 2.4yr. have been computed. 05 07.6 +09 28 STT 16 Ori. A is a spectroscopic binary. Proper motion of B +012 -013. 05 07.6 -88 52 HJ 4047 1900: 06 56.4. 05 07.8 +30 24 JOY 5 RW Aur, prototype of its class. 05 07.8 -05 05 BUP 74 Beta Eri. 05 07.9 +21 42 S 466 105 Tau. B is BD+21@764. A is a spectroscopic and occultation binary. 05 07.9 +08 30 STT 98 14 Ori. P = 199yr., a = 1.04", motion retrograde. The pair shares common proper motion with STF 643. 05 08.0 +37 03 HJ 3265 Proper motion of B -005 -002. 05 08.1 +24 16 EDG 2 103 Tau. A is a spectroscopic and occultation binary. H 114 H V 114. 05 08.9 +03 13 A 2636 P = 356yr., a = 0.36", motion direct. 05 09.3 +09 50 BUP 75 13 Ori. 05 09.6 +29 47 STT 61 Proper motion of B +056 -002. 05 09.7 +15 36 STT 99 15 Ori. Round (Hussey). May not be double. 05 09.8 +28 02 BU 1047 P = 32.1yr., a = 0.22", motion retrograde. 05 09.9 +06 05 AG 91 Proper motion of B -015 -011. 05 10.0 +37 54 SEI 81 ADS 3729a. 05 10.2 +14 00 S 468 Proper motion of B -001 -009. 05 10.2 -72 05 HJ 3746 Proper motion of B -035 -016. 05 10.3 +37 18 STF 644 One component is a spectroscopic binary. 05 10.3 -07 36 A 484 Position angles uncertain but near 130@-310@. Round 1958 with 82-inch. 05 10.5 -18 54 HJ 3727 CPD-19@760. 05 11.0 +39 17 STF 646 Proper motion of B +016 +025. 05 11.0 +32 03 STF 648 Proper motion of B -066 +045. 05 11.1 +37 18 BLL 13 B is BD+37@1072. Proper motion of B -006 -009. 05 11.5 +53 05 HJ 2251 HJ gives position angle as 319.9@. 05 11.5 -55 19 HJ 3738 B is CPD-55@759. 05 11.7 +00 31 HU 33 Round 1951, 1956. One component is a spectroscopic binary. Variable, V1085 Ori. 05 11.9 -09 07 BUP 76 B is BD-09@1093. 05 12.0 +06 50 STT 62 B is BD+06@865. Proper motion of B +029 +005. 05 12.3 -11 52 STF 655 Iota Lep. 05 12.6 -17 27 S 470 B is BD-17@1046. Proper motion of B +009 000. 05 13.3 +02 52 STF 654 Rho Ori. A is a long-period spectroscopic binary, P = 1031.4d. 05 13.5 +01 58 STT 517 P = 312yr., a = 0.38", motion direct. C may be physical. 05 13.5 -07 20 A 661 Round 1958 with 82-inch. 05 13.5 -47 53 HJ 3739 Proper motion of B -030 +044. 05 13.6 -31 54 HJ 3735 Proper motion of B +052 -069. 05 13.9 -56 48 HJ 5450 HJ 5450a. 05 14.0 +51 26 HU 821 P = 131yr., a = 0.63", motion direct. 05 14.3 +69 49 STF 638 Proper motion of B -023 -114. 05 14.3 -09 47 BRT 3264 BRT gives this as MLL 2 but position of BD-09@1103. 05 14.5 -08 12 STF 668 Rigel, Beta Ori. The companion is a spectroscopic binary and suspected visual double, although it remains unconfirmed. 05 14.5 -69 57 HJ 3754 B is CPD-70@376. 05 14.6 +76 28 HU 1097 B may be variable. 05 15.1 -36 39 HJ 3740 B is CD-36@2133. Proper motion of B -006 -004. 05 15.4 +32 41 STF 653 14 Aur. A is the Delta Scuti-type variable KW Aur, and is also a spectroscopic binary. Proper motion of B +025 -001. 05 15.5 +22 17 COU 158 108 Tau. 05 15.7 -60 00 JSP 71 JSP 71a. 05 15.8 +02 59 KU 86 Proper motion of B -008 -005. 05 16.3 +34 19 SEI 136 AE Aur. Nova remnant, probably not double. 05 16.4 -01 39 A 844 P = 178yr., a = 0.26", motion direct. 05 16.7 +46 00 ANJ 1 Aa: Capella. Composite spectrum; G5IIIe+G0III. P = 0.285yr., a = 0.055", motion retrograde. HJ 2256 AF: H VI 30. FRH 1 AH: HL is physical with AB. ST 3 The HL component at 05 17.7 +45 51 is physical. 05 16.7 +18 23 A 2430 Proper motion of B -004 -006. 05 17.2 +37 47 HJ 3271 Proper motion of B -007 +012. 05 17.2 +33 20 STF 666 Proper motion of B -001 +011. 05 17.3 +53 35 ES 2610 A is R Aurigae, variable 6.5-13.8. B is BD+53@880, F8V. Proper motion of B +051 -050. 05 17.4 +59 28 STI 561 Proper motion of B -002 -017. 05 17.5 +20 08 STF 674 A is the Algol-type binary CD Tau, P = 3.44d. B has spectral type dK2. 05 17.6 -06 51 H 25 H V 25. Tau Ori. 05 17.6 -15 13 S 473 B is BD-15@1000. Proper motion of B +018 -004. 05 17.7 +45 51 ST 3 Capella HL. See other components at 05 16.7 +46 00. A premature orbit has been computed. 05 18.2 +37 39 BU 885 BU 885 1/2. 05 18.2 +33 22 STT 103 16 Aur. A is a long-period spectroscopic binary. P = 434.8d. 05 18.7 +33 31 ES 59 Proper motion of B -006 -021. 05 18.8 -18 08 SEE 50 A is a spectroscopic binary. 05 19.1 +40 09 H 88 H V 88. Proper motion of B -085 +011. 05 19.1 +40 06 STF 3 Lambda Aur. 05 19.2 +35 48 SEI 179 A is an irregular variable, V348 Aur. 05 19.2 +20 08 STF 680 Spectrum composite; G8II-III+G1IV-V (BSC). 05 19.3 -10 45 STF 688 BDS 2665, H III 94 same star. B is BD-10@1152. Proper motion of B +041 +010. 05 19.3 -18 31 S 476 B is BD-18@1056. Proper motion of B +007 +009. 05 19.4 +40 20 SMA 50 Nothing in this position (Heintz), but probably identical to a pair at 05 18.6 +40 20. 05 19.4 +33 59 HO 18 18 Aur. 05 19.5 -30 04 HJ 3749 Proper motion of B +009 +004. 05 19.7 +25 11 STF 679 Proper motion of B +010 -063. 05 20.4 -08 02 STF 692 Proper motion of C -001 -064. 05 20.4 -33 24 HJ 3751 Proper motion of B -015 +015. 05 20.7 +46 58 STF 681 Proper motion of B -003 -017. 05 20.9 +24 02 STF 686 Proper motion of B +021 -040. 05 21.4 +33 23 ES 332 Proper motion of B +004 -015. 05 21.7 +18 54 KU 87 B is BD+18@832. 05 21.7 +12 40 STT 105 Not seen since 1971. Needs speckle. 05 21.8 +64 54 STF 659 Proper motion of B -014 -001. 05 21.8 +32 31 HU 614 A is the Mira-type variable UV Aur. 05 21.8 -24 46 HJ 3752 Spectrum composite; G7II-III+A7IV-V. 05 21.9 +42 03 AG 314 B is BD+41@1166. 05 22.0 +55 56 KR 26 Proper motion of B -008 -003. 05 22.2 +20 08 J 144 Proper motion of B -014 -016. 05 22.2 +05 24 STT 106 Proper motion of B +015 -060. 05 22.3 +33 48 STF 687 Proper motion of B -004 -009. 05 22.6 +79 14 STF 634 B is BD+79@168. Proper motion of B +055 -155. 05 22.6 +02 36 A 2641 P = 90yr., a = 1.10", motion retrograde. 05 22.8 +03 33 STF 696 23 Ori. B is BD+03@872. Proper motion of B +018 +005. 05 23.1 +31 10 STF 691 B is BD+31@947. Proper motion of B +022 -008. 05 23.1 +01 17 WEB 3 Proper motion of B -003 +001. 05 23.1 +01 03 STF 700 Proper motion of B +046 -061. 05 23.4 +49 34 ES 2614 Proper motion of B -002 -056. 05 23.5 +57 33 BU 1393 16 Cam. A is a spectroscopic binary. 05 23.5 +16 02 STF 697 B is BD+15@804. Proper motion of B +004 -010. 05 23.9 -00 52 WNC 2 A-BC: A is a spectroscopic binary. A-BC is physical. A 847 BC: Ambiguous case; P = 24.7 or 46.3yr., a = 0.19 or 0.34", inclination 82 or 90 degrees. 05 24.4 +17 23 S 478 111 Tau. A is a spectroscopic binary. B is BD+17@919. Proper motion of B +027 -019. 05 24.5 -02 24 MCA 18 Eta Ori. A is a spectroscopic and eclipsing binary, P = 7.99d. A has been resolved into a third component by speckle interferometry. A spectroscopic period of 9.51y has been determined. H 67 H VI 67. 05 24.6 +09 10 A 2703 Too close 1937, 1951, 1954. 05 24.6 +01 49 S 479 B is BD+01@1003. Proper motion of B +007 +007. 05 24.7 +63 23 STF 677 P = 340yr., a = 1.50", motion retrograde. 05 24.7 +37 23 BU 888 Sigma Aur. 05 24.8 -52 19 I 345 Theta Pic. A is a spectroscopic binary. 05 25.0 -02 49 H 68 H IV 68. B is BD-02@1238. 05 25.1 +06 21 BUP 78 Gamma Ori. 05 25.2 +34 51 STF 698 Spectrum composite; K1pIII-IV+F6V. B is BD+34@1030. Proper motion of B -011 -051. 05 25.2 -11 19 STF 710 B is BD-11@1168. 05 25.5 -00 33 A 848 P = 339yr., a = 0.24", motion direct. 05 25.6 +38 03 STF 699 Proper motion of B +000 -018. 05 25.6 +36 52 SEI 246 Nothing at this position (Heintz). 05 25.6 -60 05 HJ 3764 CD-60@1161. 05 25.9 -35 21 HJ 3760 Proper motion of B +015 -033. 05 26.0 -19 42 HJ 3759 B is BD-19@1172. Proper motion of B -001 -039, spectrum F5/7V. 05 26.3 +28 36 BAR 26 Beta Tau. 05 26.4 -43 23 HJ 3763 B is CD-43@1846. Proper motion of B +027 +001. 05 26.8 +57 48 STF 690 Proper motion of B +018 +020. 05 26.8 +03 06 KNT 3 Psi (2) Ori. A is a variable, P = 2.52d. a spectroscopic binary. 05 26.9 +37 06 COU 1725 A variable, W Aur. 05 27.1 +34 10 BLL 14 A is a semiregular variable, S Aur. 05 27.2 +17 58 MCA 19 115 Tau. A is an occultation binary which has been resolved by speckle interferometry. 05 27.6 +34 29 BUP 79 Phi Aur. D is BD+34@1049. 05 27.6 +21 56 HJ 365 114 Tau. A is an occultation binary. 05 27.6 -00 38 BAL 670 Proper motion of B -007 -037. 05 27.6 -20 55 SEE 53 P = 117yr., a = 0.26", motion direct. 05 27.6 -61 20 JSP 79 CD-61@1111. 05 28.1 +40 21 ES 2615 B is BD+40@1296. Proper motion of B 000 -015. 05 28.2 +02 23 J 49 Too close 1951 with probable quadrant change (van Biesbroeck). Round in 1990. Needs speckle. 05 28.2 -01 56 HJ 702 Proper motion of B +001 -004. 05 28.2 -20 46 BU 320 Beta Lep. Proper motion of B -004 -089. 05 28.4 +86 05 STF 573 B is BD+85@71. Proper motion of B -023 +032. 05 28.7 -65 27 RST 137 AB Dor, a rapidly rotating, spotted star which shows both X-ray flares and microwave emission. 05 28.9 +67 55 STF 689 Proper motion of B -014 +012. 05 29.0 -04 42 WEB 4 A is the Mira-type variable S Ori. Proper motion of B +066 -022. B is -04@1144. 05 29.1 -02 01 D 8 Proper motion of B +020 -030. 05 29.2 +38 48 BU 1318 Proper motion of B -002 -014. 05 29.3 +25 09 STF 716 118 Tau. 05 29.4 +11 52 HER This is the T-Tauri variable V649 Ori. 05 29.4 -07 16 H 101 H V 101. 05 29.6 +33 50 ES 282 Not found by Heintz. 05 29.6 +30 45 KU 88 B is BD+30@910. Proper motion of B -020 -036. 05 29.7 +35 23 HU 217 A is the Beta Lyrae-type system, LY Aur, P = 4.00d. 05 29.7 +33 27 S 484 B is BD+33@1063. Proper motion of B +021 -038. 05 29.7 -01 06 STF 725 31 Ori. A is the variable CI Ori. Proper motion of B +029 -030. 05 30.1 -32 28 B 1946 Not seen for certain 1951-1967. 05 30.2 +41 45 A 1720 A measure by A 1907.8, 259@, 1.9". 05 30.3 -23 31 B 2587 Spectrum: Fm Delta Del. 05 30.8 +39 50 STT 63 B is BD+39@1321. Proper motion of B +013 -019. 05 30.8 +05 57 STF 728 32 Ori. A premature orbit has been computed. The motion is nearly rectilinear. 05 30.8 -00 22 A 852 Appears to be in rapid motion. This is the variable V1093 Ori. 05 30.8 -12 51 BRT 2644 RST 3426. BRT identifies this as BD-12@1187. 05 30.8 -70 55 HJ 3783 Proper motion of B -045 +018. 05 30.9 +01 37 BAL 1294 Proper motion of B -007 +013. 05 31.1 +42 55 A 1721 Too close 1924-1931(Aitken). This interval may mark a quadrant change. 05 31.2 +03 18 STF 729 33 Ori. Proper motion of B -001 +003. 05 31.2 -42 19 DUN 22 Proper motion of B +041 -008. 05 31.4 -03 36 ENG 20 Proper motion of A +774 -2090. B is BD-03@1122. 05 31.5 +54 39 STF 711 Proper motion of B -132 -353. 05 31.7 +02 50 SHJ 61 Proper motion of B -004 +005. 05 31.9 -76 20 HJ 3795 Gamma Men. 05 32.0 -00 18 HEI 42 Delta Ori. A is an Algol-type system, as well as a close visual binary. STF 14 C is a spectroscopic binary. 05 32.1 -05 06 DOO 34 DOO identifies this as BDS 2801, but evidently it is a different pair. 05 32.2 +70 49 A 1034 P = 400yr., a = 0.70", motion retrograde. 05 32.2 +17 03 STF 730 A is a spectroscopic binary. Proper motion of B -001 -003. 05 32.3 +02 17 A 2509 Not seen 1913-1936, when about 100@ of orbital motion took place. 05 32.4 -06 24 ENG 21 B is BD-06@1211. 05 32.7 -01 36 BU 1048 A is variable. 05 32.7 -17 49 HJ 3766 Alpha Lep. 05 33.0 -24 15 DAW 85 P = 60.6 or 89.3yr., a = 0.31 or 0.34", motion retrograde. 05 33.1 +02 28 AG 96 Proper motion of B -019 -011. 05 33.5 +16 01 STF 733 Proper motion of B -007 -019. 05 33.6 -51 04 HU 1566 P = 281yr., a = 1.27", motion retrograde. 05 34.1 +69 40 STF 704 Proper motion of B +015 -006. 05 34.1 -01 02 H 118 H V 118. 05 34.2 +10 19 LDS 6189 This is the common proper motion pair Ross 45. 05 34.3 +36 03 SEI 326 Identified as BD+35@1169. Possibly BD+35@1168. 05 34.8 +09 29 MCA 20 Phi (1) Ori. This speckle observation probably repre- sents the known spectroscopic binary with P = 8.4yr. 05 34.9 -00 07 STF 741 Proper motion of B +009 +038. 05 35.0 +15 44 HEI 43 Heintz reports a third star at 283 degrees, 40". 05 35.0 -06 00 STF 747 B is BD-06@1233. Proper motion of B +005 -002. 05 35.1 +09 56 STF 738 Lambda Ori. 05 35.2 +10 14 STT 111 The primary is a single-lined spectroscopic binary, P = 1857d. 05 35.2 -46 57 RST 141 P = 85yr., a = 0.28", motion direct. 05 35.3 -05 23 STF 748 Theta (1) Ori. A is an Algol-type system, V1016 Ori. B is an Algol-type system, BM Ori. C is a RW Aur-type system, V361 Ori. Common proper motion with the mul- tiple system STF 16. 05 35.4 -04 50 DA 4 42 Ori. 05 35.4 -05 25 STF 16 Theta (2) Ori. B is BD-05@ 1320. Proper motion of B +013 +015. A is a spectroscopic binary, P = 21d. 05 35.4 -05 55 STF 752 Iota Ori. A is a spectroscopic binary, P = 29.1d. 05 35.5 -05 25 S 490 Variable, V361 Ori. 05 35.7 -04 51 HLD 173 45 Ori. 05 35.8 -00 59 STF 751 B is BD-01@966. Proper motion of B +001 +002. 05 35.9 -05 38 DA 3 A is a spectroscopic binary and light variable. 05 36.2 -01 12 BUP 81 Epsilon Ori. Possibly variable. 05 36.2 -13 49 WEI 9 B is BD-13@1193. 05 36.4 +34 08 STF 737 B is BD+34@1106. Proper motion of B +001 -003. 05 36.4 +22 00 STF 742 Proper motion of B -060 -105. A premature orbit has been computed. 05 36.5 -06 43 J 798 Center of nebula H IV 33 (Jonckheere). AC: Did not find Jonckheere component (Couteau, 1960). The two componnents may in fact be the same. The A component is the RW Aur-type variable V380 Ori. 05 36.6 -06 04 STF 754 A is a spectroscopic binary. 05 36.7 -69 30 I 1151 An S Doradus-type variable, R127, in the LMC. 05 37.3 +66 42 MLR 314 P = 41yr., a = 0.22", motion direct. 05 37.3 +64 09 HU 1107 19 Cam. 05 37.6 +02 19 STF 756 Proper motion of B -022 -012. 05 37.7 -53 30 HJ 3786 Spectrum of A is F/G. 05 37.8 -54 34 HJ 3787 B is CPD-54@866. 05 38.4 +43 01 A 1563 Less than 0.1" with 82-inch 1953, 1954. A premature orbit has been computed. 05 38.6 +30 30 BU 1240 26 Aur. P = 53yr., a = 0.14", motion retrograde. Composite spectrum; B9.5V+F9III. 05 38.6 -02 33 STF 761 AB: B is BD-02@1324. Rabe measures principal stars STF 761 and STF 762. 1914, 324@, 209.79". 05 38.6 -41 18 HJ 3781 Proper motion of B -012 -021. 05 38.7 -02 36 BU 1032 Sigma Ori. P = 155.3yr., a = 0.264", motion retrograde. A is variable, V1030 Ori. This is a trapezium system with at least five components, including the helium- rich star E , BD-02@1327. A has also been reported to be a short period, double-lined spectroscopic binary. 05 39.1 -50 08 HJ 3789 B is CD-50@1871. 05 39.2 +23 17 STF 755 Proper motion of B +027 -059. C is a spectroscopic binary. 05 39.3 +10 16 STF 763 Proper motion of B -001 -013. 05 39.4 +43 43 A 1564 P = 187yr., a = 0.20", motion direct. 05 39.5 +53 52 AG 316 Proper motion of B -014 +019. 05 39.6 -34 04 HDO 193 Alpha Col. 05 39.9 +51 45 ES 893 Proper motion of B +002 -001. 05 40.3 +15 21 STF 766 Proper motion of B +012 -035. 05 40.7 -01 57 STF 774 Zeta Ori. A premature orbit has been computed. Variable radial velocity of A not confirmed. C may be physical. Spectral types of AB: O9.5Ibe and B0III. 05 41.3 +29 29 STF 764 A is a spectroscopic binary. B is BD+29@954. Proper motion of B +019 -028. 05 41.3 +16 32 BU 1007 126 Tau. P = 115yr., a = 0.33", motion direct. The variable radial velocity indicates a spectroscopic subsystem. 05 41.3 -26 21 HJ 3788 B is CD-26@2394. Proper motion of B -133 +004. 05 41.7 -02 54 BU 1052 P = 107.5yr., a = 0.39", motion retrograde. 05 42.1 +32 45 HJ 369 Measure does not agree with HJ, but so identified by Doolittle. 05 42.4 +79 20 STF 695 Proper motion of B -006 -042. 05 42.5 +40 53 WEI 10 B is BD+40@1384. Proper motion of B -002 -005. 05 42.8 +65 08 MLB 339 Proper motion of B -008 -005. 05 42.9 +00 01 STF 782 B is BD-00@1060. Proper motion of B +010 -023. 05 42.9 -06 48 A 494 P = 20yr., a = 0.20", motion direct. 05 43.4 +22 13 STF 777 Proper motion of B 000 +012. 05 43.5 -07 53 A 495 Angle decreasing. No measures 1963-1988, during which period nearly two quadrants were described. 05 43.6 +66 33 HU 1109 A is reported to be variable, type unknown. 05 43.6 +13 00 A 117 A 14.5 magnitude star is 26" from A in 191@. 05 44.1 -02 29 A 2918 B is BD-02@1354. Proper motion of B +002 -009. 05 44.4 +27 44 STF 779 Proper motion of B -028 -028. 05 44.5 -22 27 H 40 AB: H VI 40. Gamma Lep. Proper motion of B -304 -358. H 50 BC: H V 50. C is CPD-22@883. 05 44.7 +03 50 STF 788 Proper motion of B -020 +008. 05 44.7 -46 18 HJ 3797 B is CD-46@1983. 05 45.0 +04 00 STF 789 Proper motion of B -005 +008. 05 45.6 -15 03 ENG 23 B is BD-15@1153. Proper motion of B -016 +016. 05 45.9 +25 55 STF 785 Proper motion of B +012 -015. 05 46.0 +10 48 A 2711 May be a short period binary, but the few measures do not even permit certain determination of the direction of motion. 05 46.0 -04 16 STF 790 Composite spectrum; K1III+G0IV. 05 46.3 +37 36 GCB 66 A is the short-period variable EU Tau. 05 46.9 +09 31 J 251 Proper motion of B -006 -031. 05 47.0 -44 48 HJ 3803 Proper motion of B -004 -019. 05 47.2 +21 53 HU 39 Measures scattering around 45 degrees, with variation in distance evident. Motion in a highly-inclined orbit? 05 47.2 +14 29 CHR 160 131 Tau. 05 47.2 -24 30 HJ 3798 B is CD-24@3430. Proper motion of B +003 +040. 05 47.3 +32 22 J 902 This pair is 1.36s f and +30.7" nf of BD+32@1087. 05 47.4 +28 58 HJ 709 First distance probably in error (Doolittle). 05 47.4 -10 32 MCA 22 An eclipsing binary and spectroscopic triple, V1031 Ori, with the wider pair, presumably, now resolved by speckle interferometry. 05 47.6 +17 36 BU 1401 Probably STF 767 rej. 05 47.7 +13 54 HJ 3279 133 Tau. 05 47.9 +24 41 STT 66 B is BD+24@965. Proper motion of B +004 -001. 05 48.0 +06 27 STF 795 52 Ori. One component is a spectroscopic binary. 05 48.2 +01 37 A 2657 P = 60yr., a = 0.13", motion direct. 05 48.4 +20 52 STT 118 A is a spectroscopic binary. A premature visual orbit has been computed. 05 48.8 -65 52 HJ 3815 B is CPD-65@506. 05 48.9 +21 01 BU 93 B is BD+20@1112. Proper motion of B -013 -012. 05 49.0 +24 34 MCA 23 132 Tau. 05 49.1 -61 08 HJ 3810 B is CPD-61@532. 05 49.2 +39 11 BU 192 Tau Aur. 05 49.5 +12 39 BUP 84 134 Tau. 05 49.6 -14 29 BU 94 BDS 3207 probably same star. 05 49.7 -04 27 SCJ 3 B is BD-04@1249. 05 49.8 +32 58 S 500 B is BD+32@1099. Proper motion of B +012 +007. 05 49.8 +06 05 HJ 712 Proper motion of B -006 -005. 05 50.3 +04 17 BAL 2643 Proper motion of B -005 -015. 05 50.5 -52 46 B 1493 Spectrum composite; K0-1III+A4V+A. 05 50.6 +56 55 H 125 H IV 125. 29 Cam. 05 50.8 -01 16 BAL 312 Proper motion of B -024 -001. 05 51.0 +27 58 BU 1054 136 Tau. A possible occultation binary. 05 51.0 -69 54 HJ 3820 B is CPD-69@535. 05 51.4 +35 35 HJ 710 Points to a 14th magnitude star 30". 05 51.4 +32 07 ES 415 A is variable. 05 51.5 +39 09 H 90 H V 90. Nu Aur. 05 51.8 +28 27 STF 805 Proper motion of B +021 -010. 05 51.8 +10 26 AG 319 Proper motion of B -018 +008. 05 52.3 +12 53 COU Couteau calls this AD, but the magnitude for A is wrong if this is AD. 05 52.4 +01 51 BU 1404 56 Ori. 05 52.5 +15 48 BID 1 A is a Mira-type variable, Z Tau. 05 52.8 +29 46 D 10 Proper motion of B +031 -063. 05 53.1 +41 27 ARG 61 B is BD+41@1290. 05 53.3 +27 37 BU 1054 Possibly an occultation binary. 05 53.5 +42 49 ARG 62 Proper motion of B -011 -007. 05 53.6 -03 36 B 2592 A faint pair 10s p 3' s. 05 53.8 -22 18 BRT 1382 CD-22@2561. 05 54.2 -29 09 FIN 382 Angle decreasing. 05 54.3 -25 53 I 1614 B is CD-25@2770. Proper motion of B -009 -004. 05 54.4 +38 36 WEI 11 B is BD+38@1326. Proper motion of B +020 -002. 05 54.6 +05 21 STF 815 Proper motion of B -013 -005. 05 54.7 +13 51 S 502 B is BD+13@1027. Proper motion of B +001 -006. 05 54.9 +07 02 STF 817 Proper motion of B +011 -006. 05 55.1 -00 56 STF 819 Proper motion of B -026 -005. 05 55.2 +07 24 KAR 1 H VI 39. Alpha Ori. An irregular variable, spectrum M1-2Ia-Iab. Two close companions have been reported, detected by speckle interferometry. 05 55.3 +04 43 STF 818 Proper motion of B -020 -037. 05 55.6 +53 28 STT 120 B is BD+53@963. Proper motion of B -014 -041. 05 55.7 +08 59 STF 820 Proper motion of B -022 +000. 05 55.8 +36 56 STT 122 P = 220 yr., a = 0.40", motion direct. 05 55.9 +14 00 S 503 Proper motion of B -044 +008. 05 57.1 +10 14 ARG 63 B is BD+10@939a. Proper motion of B -019 -003. 05 57.3 +38 51 ES 2153 ADS 4527a. 05 57.3 -27 20 HJ 3818 Spectrum: G8/K0IIICNpv. 05 57.5 -35 17 HJ 3819 Gamma Col. 05 58.0 -52 12 HU 1570 P = 190yr., a = 0.59", motion direct. 05 58.4 +01 50 H 100 H V 100. 59 Ori. A Delta Scuti-type variable, V1004 Ori, Ori, and also a spectroscopic binary. Proper motion of B +003 +007. 05 58.5 -20 10 S 504 Proper motion of B +034 +012. 05 58.8 +00 33 KUI 22 60 Ori. A is a spectroscopic binary. 05 58.9 +12 48 STT 124 P = 140yr., a = 0.30", motion direct. 05 59.5 +58 53 ES 66 ES 66a. 05 59.5 +54 17 ENG 24 Delta Aur. 05 59.5 +44 57 H 88 H VI 88. Beta Aur. An Algol-type system, P = 3.96d. 05 59.7 +37 13 STT 545 Theta Aur. A is a variable of the Alpha CVn type. 06 00.3 +44 36 BU 1055 Composite spectrum; K2III+K0III. H 91 AC: H VI 91. 06 00.3 -31 02 HU 1399 P = 72yr., a = 0.94", motion retrograde. HJ 3823 AB-C: A premature orbit has been computed. 06 00.7 -02 04 RST 4290 Proper motion of B +001 -005. 06 01.0 +27 34 SMK 1 Resolved by two occultation events at favorable aspects. 06 01.1 +23 20 H 48 H IV 48. 06 01.8 -10 36 BU 16 3 Mon. A is a spectroscopic binary. 06 01.8 -41 10 HJ 3827 CPD-41@872. 06 02.2 +00 59 HJ 2290 Proper motion of B -007 -013. 06 02.4 +09 39 A 2715 Mu Ori. P = 18yr., a = 0.28", motion retrograde in a highly-inclined orbit. A is a variable of the Alpha CVn type, and a spectroscopic binary, P = 4.45d. 06 03.0 +09 45 MLL 10 Probably identical with ADS 4627, J 1323. 06 03.2 +58 13 A 1315 A premature orbit has been computed. 06 03.4 +27 38 STF 830 Proper motion of B +009 +017. 06 03.5 +19 41 MCA 24 64 Ori. A spectroscopic binary and occultation triple, with the wider pair, presumably, now resolved. Fekel and Scarfe (Astron. J. 92, 1162; 1986) report periods of 14.57d and 13.03yr. 06 03.6 +04 19 STF 837 Identical with STF 833 rej. BAL 2649. Proper motion of B +007 -033. 06 04.1 +23 16 KUI 23 1 Gem. B is a spectroscopic binary, P = 9.6d, and A is reported to be an occultation binary. Evidently both visual components are giants with one, probably the later type component, double once more. AB: P = 13.35yr., a = 0.20", motion direct. 06 04.5 +51 34 STT 128 Possibly variable. 06 04.6 +30 14 STF 834 B is BD+30@1097. 06 04.8 -48 28 DUN 23 P = 464yr., a = 2.94", motion direct. Variable? 06 04.9 -05 21 H 14 H V 14. 06 05.1 +00 53 STF 838 Proper motion of B +009 -005. 06 05.2 -14 19 STF 843 Position corrected. 06 05.3 +74 00 STT 121 P = 163yr., a = 0.41", motion retrograde. 06 05.5 +14 35 AG 321 Proper motion of B -003 -012. 06 05.9 +48 15 ES 1234 The primary is a double-lined spectroscopic binary. 06 06.1 +35 23 ENG 25 B is BD+35@1335. 06 06.5 +10 45 STF 840 Proper motion of B +013 -021. 06 06.6 +04 31 VBS 12 The primary is Ross 413. 06 07.1 +41 46 MLB 1065 Proper motion of B +003 -075. 06 07.4 +02 09 STF 846 Proper motion of B +012 -002. 06 07.5 -22 44 DON 1065 CD-22@2776. 06 07.9 +28 58 HJ 378 Proper motion of B +030 -001. 06 07.9 -42 09 FIN 70 Pi (2) Col. Position angle uncertain. Many attempts, but few successful observations. Needs speckle. 06 08.1 -25 25 B 99 Last position angle uncertain. Not resolved by Finsen in 1960-62. Motion retrograde. 06 08.3 +14 00 STF 844 Proper motion of B +011 -026. B is BD+14@1161. 06 08.5 +05 48 STF 854 Proper motion of B -003 -022. 06 08.6 +05 48 STF 852 BD+07@1145a. 06 09.0 +02 30 STF 855 B is BD+02@1140. 06 09.1 +07 03 STF 856 Proper motion of B -003 -004. 06 09.2 +11 39 STF 853 Proper motion of B -026 -018. 06 09.3 +28 39 A 121 164" in 247@ from BD+28@1026. 06 09.3 +24 26 STT 134 Proper motion of B -006 +002. 06 09.4 +34 28 HJ 380 Proper motion of B +003 -019. 06 09.6 +05 40 STF 859 B is BD+05@1116, proper motion -002 -038. 06 09.7 +43 08 WEB 5 B is BD+43@1465. Proper motion of B +004 -003. 06 09.7 +23 07 BU 1241 3 Gem. B is variable. 06 09.8 -22 46 RST 3442 P = 18.21yr., a = 0.206", motion direct. 06 10.3 +15 54 H 114 H VI 114. 06 10.5 +23 00 BU 1058 4 Gem. 06 10.7 -09 51 STF 869 B is BD-09@1351, and is reported to be a variable of unknown type. Proper motion of B +027 +014. 06 10.9 +10 20 KAM 1 Ross 79. 06 11.1 +67 59 STF 831 Proper motion of B +013 +004. 06 11.5 +57 02 ARG 13 B is BD+57@944. 06 11.6 +48 43 STF 845 41 Aur. Proper motion of B +010 -070. 06 11.6 -00 46 STF 871 Proper motion of B +002 -010. 06 11.7 +01 46 BAL 1305 Proper motion of B -010 -022. 06 11.7 -04 40 AC 3 A variable, V638 Mon. 06 11.9 +14 13 J 2016 Xi Ori. A is a spectroscopic binary, P = 45.1d. 06 12.0 +19 47 CHR 163 68 Ori. B is BD+19@1252. H 72 is H VI 72. Proper motion of B +127 -142. 06 12.0 -74 31 HJ 3855 Proper motion of B -003 -033. 06 12.2 -65 32 DUN 26 B is CPD-65@566. Proper motion of B 000 +136. 06 12.4 +23 59 J 1102 Single 1958, 1960 (Couteau). Probable positional error. 06 12.6 -01 18 STF 873 Proper motion of B +002 -002. 06 13.0 -22 03 BRT 304 CD-22@2857. 06 13.7 -00 19 BAL 686 Proper motion of B +002 -123. 06 14.1 +23 59 STT 70 B is BD+23@1258. proper motion of B -001 +006. 06 14.3 +14 30 S 509 B is BD+14@1210. 06 14.5 +17 54 KUI 24 A spectroscopic binary. 06 14.5 +11 48 STT 71 B is BD+11@1075. Proper motion of B -005 -010. 06 14.5 -45 21 CPO 133 B is CD-45@2390. 06 14.7 +14 35 STF 877 B is a spectroscopic binary. 06 14.7 +07 14 BRT 2115 Possibly J 1933 with erroneous measure. 06 14.8 +19 09 HJ 2302 71 Ori. 06 14.9 +22 30 BU 1008 Eta Gem. A is a semi-regular variable. A premature visual orbit has been computed. A is also an occulta- tion binary and a long-period spectroscopic binary. 06 14.9 -06 17 HJ 384 Gamma Mon. 06 15.1 +44 10 KU 90 Proper motion of B +013 -009. 06 15.4 -09 02 A 668 P = 107.2yr., a = 0.201", motion direct. 06 15.5 +10 35 STF 880 Proper motion of B +000 -015. 06 15.6 +66 09 STT 69 BC is BD+66@436. MLR 316. Proper motion of B -001 -029. 06 15.6 +36 09 STF 872 AB: Proper motion of B -076 +012. 06 15.7 +60 00 BUP 86 40 Cam. 06 15.8 +66 08 MLR 316 See STT 69 at 06156. 06 15.9 +01 10 RST 5225 P = 30yr., a = 0.17", motion direct. 06 16.3 -59 13 DUN 27 B is CPD-59@618. 06 16.4 +12 16 KUI 26 74 Ori. 06 16.7 +38 52 J 591 Single 1931 (Giacobini). Position may be erroneous. 06 16.9 +06 00 STF 885 Proper motion of B -007 -010. 06 17.1 +15 51 H 23 H V 23. B is BD+15@1138. 06 17.1 +09 57 FIN 331 75 Ori. Aa: P = 9.20yr., a = 0.090", motion direct. 06 17.2 +33 12 COU 1406 The variable VW Aur. 06 17.3 +05 06 ENG 26 B is BD+05@1165. 06 17.8 +26 12 AG 322 B is BD+26@1167. Proper motion of B 000 -035. 06 18.3 +62 12 STF 866 Proper motion of B -010 -015. 06 18.6 +67 44 HU 1119 P = 200yr., a = 0.72", motion direct, highly-inclined. 06 18.6 -29 22 I 1116 Spectrum: A2(m)A7/8-F2. 06 19.2 +14 48 HJ 3281 Woods measures this pair 1909.98, 262.4@, 5.72". Another pair? 06 19.3 -12 32 HO 231 This pair was listed as HJ 3847, but with an error of two degrees in declination. 06 19.3 -24 58 S 516 AB: B is CD-24@3914. Proper motion of B +015 -031. 06 19.4 +23 16 H 55 H V 55. 06 19.4 +13 26 STT 73 B is BD+13@1200, and is a spectroscopic binary. Proper motion of B +012 -014. 06 19.7 -07 49 CHR 22 7 Mon. 06 19.8 -39 30 HJ 3849 B is CD-39@2525. Proper motion of B +003 -011. 06 20.0 +28 26 BU 895 Ambiguous case: P = 54 or 108yr., a = 0.18 0r 0.28", motion direct. 06 20.0 -10 38 A 2925 Apparently a rapid binary, distance 0.3" or less. Single 1958, 1974-75. In the "red rectangle", a bi-polar nebula. 06 20.3 -29 37 JC 3 Proper motion of B +079 +049. 06 20.3 -30 04 SMY 1 Zeta CMa. A is a long-period spectroscopic binary. P = 675d. B is CD-29@3008. Proper motion of B -004 +011. 06 20.4 +29 40 BRT 3273 Barton calls this RMK 4, and this is copied in ADS. But RMK 4 is properly CPD-57@659. Proper motion of B +010 -017. 06 20.6 +25 11 STT 74 B is BD+25@1222. Proper motion of B +005 -002. 06 20.6 +18 03 STT 75 B is BD+18@1179. Proper motion of B -002 -018. 06 20.8 +08 49 J 409 Proper motion of B -018 -027. 06 20.8 +05 44 STF 895 Proper motion of B -007 -002. 06 21.4 +02 16 A 2667 P = 99yr., a = 0.40", motion direct. One component variable? 06 21.4 -11 46 STF 3116 A is a Cepheid, FR CMa. 06 21.7 +36 07 STF 890 B is CPD-59@618. 06 21.9 +54 59 ES 2617 Proper motion of B +008 +023. 06 22.1 +59 22 CHR 128 4 Lyn. 06 22.4 +26 40 STF 897 Proper motion of B -006 +004. 06 22.4 +21 59 L 37 L measured an unidentified pair near this position: 1910.2, 120@, 1.22", 9.0-9.5. 06 22.7 -17 57 BUP 88 Beta CMa. Prototype of its class of variable. B is BD-17@1466. 06 23.0 +22 31 BU 1059 Mu Gem. A is an irregular variable. 06 23.3 -00 57 BAL 698 Proper motion of B -015 +005. 06 23.5 +14 33 J 1254 A is an Algol-type system, FI Ori. 06 23.6 +17 39 A 2517 Round 1952, 1955, 1983. 06 23.8 +04 36 STF 900 Epsilon Mon. A is a spectroscopic binary, P = 331d? B is BD+04@1237. Proper motion of B +034 -068. 06 23.8 -09 21 A 669 Too close 1941 and 1951. Rapid binary. 06 24.0 -21 37 B 2110 CPD-21@1254. 06 24.2 +73 55 STF 868 Proper motion of B -004 +004. 06 24.4 -16 13 S 518 B is BD-16@1468. 06 24.7 -05 44 HJ 38 BDS gives 1900: 06h 17.9m, -05@40'. 06 24.9 +31 50 AG 111 Proper motion of B -007 -015. 06 25.5 +23 20 MCA 26 An occultation and interferometric binary. 06 25.6 +22 27 STT 139 P = 514yr., a = 0.75", motion direct. 06 25.8 +36 27 BRT 3245 ALI 323. A is an irregular variable, KS Aur. 06 25.9 +51 53 STF 896 B is BD+51@1189. Proper motion of B +003 -007. 06 26.2 +18 45 BU 1191 A is a spectroscopic binary, P = 6.99d. It is also one of the brightest BY Dra-type variables known, OU Gem. 06 26.6 -21 08 B 2113 CPD-21@1283. 06 26.7 -07 31 STF 914 BDS 3401 probably same star. B is BD-07@1428. Proper motion of B -006 -013. 06 26.8 +58 25 S 514 5 Lyn. A is a spectroscopic binary. 06 26.9 +04 04 STF 911 Proper motion of B +008 +015. 06 27.4 -25 44 B 114 P = 59.7yr., a = 0.38", motion direct. 06 27.5 +34 57 STF 902 Proper motion of B +011 -005. 06 27.5 +24 32 AG 112 Proper motion of B +031 -024. 06 27.6 -25 24 BRT 2874 CPD-25@1447. 06 27.8 +20 47 SHJ 70 B is BD+20@1426. Proper motion of B -010 -016. 06 28.0 -04 46 BUP 89 10 Mon. 06 28.2 +05 16 STF 915 Variable, V648 Mon. Proper motion of B -025 -015. 06 28.4 +31 16 AG 113 Proper motion of B -025 -060. 06 28.4 +08 34 AG 114 Proper motion of B -004 -007. 06 28.4 -04 28 J 1949 B is BD-04@1533. 06 28.6 -78 54 HJ 3888 B is CPD-78@233. 06 28.7 +35 16 STF 909 Proper motion of B +037 +010. 06 28.7 -32 22 BU 753 Variable. 06 28.8 -07 02 STF 919 Beta Mon. A,B, and C are shell stars. 06 29.0 +20 13 STT 77 Nu Gem. BU 1192 BC: Round 1955 (Van Biesbroeck and Finsen) but uncertain whether measures pertain to BC or Aa. BTZ 1 Aa: Probably a spectroscopic binary, now resolved. P = 11.7yr., a = 0.05", motion direct. 06 29.1 -40 22 DUN 29 B is CD-40@2487. Proper motion of B -011 -011. 06 29.3 -02 48 B 2601 Ross 614. Possibly first resolved by van den Bos. P = 16.6yr., a = 0.93", motion direct. A is the flare star, V577 Mon., and B is also a flare suspect. 06 29.6 +72 58 HJ 2309 See note in ADS. 06 29.8 -50 14 R 65 AB: P = 52.9yr., a = 0.48", motion retrograde. A is a spectroscopic binary. HDO 195 CD: P = 101 yr., a = 0.51", motion direct. 06 29.9 +07 07 STT 142 The primary is a spectroscopic binary. The pair formerly listed as J 2004 appears to be identical, with distance doubled. 06 30.2 -22 28 BRT 1388 CD-22@3140. 06 30.5 +04 20 STF 920 Proper motion of B -004 +004. 06 30.7 +20 25 H 111 H N 111. 06 30.8 +58 10 STT 6 Lyn. B is BD+58@933. 06 31.1 +66 38 MLB 398 Proper motion of B +006 -038. 06 31.1 +21 43 WEI 12 BDS 3400, H N 141 same star. Proper motion of B -002 -005. 06 31.2 +16 56 STT 143 A is a spectroscopic binary. 06 31.2 +11 15 STF 921 B is BD+11@1205. Proper motion of B +013 +004. 06 31.3 +04 50 BAL 2666 Proper motion of B -008 -010. 06 31.4 +07 49 A 2817 P = 31.6yr., a = 0.20", motion direct. 06 31.6 +04 51 BAL 2667 Proper motion of B -012 +006. 06 31.7 +05 46 STF 926 Proper motion of B +011 -009. 06 31.9 +04 57 GAN 3 A is a Beta CMa-type variable. 06 31.9 -09 38 A 670 Rapid direct motion. 06 31.9 -23 25 SEE 68 Zeta (1) CMa. A is a Beta CMa-type variable. 06 31.9 -32 45 JSP 105 CPD-32@1200. 06 32.0 -58 45 HJ 3874 Mu Pic. 06 32.1 +04 58 H 37 H II 37. Proper motion of B -013 -011. 06 32.1 +01 30 BAL 1315 Proper motion of B +001 -002. 06 32.3 +52 25 WOR 6 P = 37yr., a = 0.52", motion retrograde. 06 32.3 +17 47 STF 924 BDS 3424 probably same star. Spectrum of B: F6IV/V. The A component is an occultation double. Proper motion of B +043 +028. 06 32.4 +13 12 AG 326 1894: No companion seen. 1903: Probably double but too close to measure. Heintz finds a faint companion at 4@, 12th mag., which does not fit the AG description. 06 32.4 +03 29 J 982 Proper motion of B -007 -005. 06 32.5 -19 46 B 1959 CPD-19@1324. 06 32.6 -32 02 HJ 3869 Proper motion of B +005 +007. 06 32.8 +10 10 ABT 5 Proper motion of B +004 -011. 06 33.2 +25 17 HJ 392 B is BD+25@1318. Proper motion of B -016 -009. 06 33.6 -12 07 HU 43 Position and BD number corrected by Heintz. 06 34.1 +22 07 S 524 B is BD+22@1384. Proper motion of B -003 -045. 06 34.2 +07 59 STF 930 Proper motion of B -474 +003. 06 34.3 +38 05 STT 147 B is BD+38@1524. Proper motion of B +024 -010. 06 34.4 +14 45 STF 932 A premature orbit has been computed. 06 34.5 -11 14 HO 234 P = 162yr., a = 0.43", motion direct. 06 34.8 +07 34 STF 938 14 Mon. 06 34.8 -06 10 A 507 AB-C: This connects the pair to BD-06@1616. 06 35.6 -62 38 FIN 74 Nova Pictoris, RR Pic. Observations of the ejecta simi- lar to those made by Kuiper for Nova Herculis (1934). Not a double star. 06 35.7 -41 29 I 1154 I 1154 1/2. 06 35.9 +05 19 STF 939 B is BD+05@1317. Spectrum of A: B0.5III-IV. Proper motion of B +002 +014. 06 35.9 -09 27 HJ 734 Proper motion of B -008 -009. 06 35.9 -36 05 FIN 19 P = 29yr., a = 0.30", motion retrograde. 06 36.0 -22 37 BRT 1390 CD-22@3251. 06 36.1 -24 07 ARG 15 B is CD-24@4208. Proper motion of B -049 -021. 06 36.4 +30 06 A 217 Single 1927-1954 (Van Biesbroeck) 06 36.4 +27 17 STT 149 P = 121yr., a = 0.89", motion retrograde. 06 36.4 +21 04 J 1101 Single 1954 (Couteau, 15-inch). 06 36.4 -18 40 SHJ 73 H IV 81. Nu (1) CMa. Composite spectrum; G8III+F3IV-V. B is BD-18@1478. Proper motion of B -026 +035. 06 36.5 +38 27 BLL 17 A is the semiregular variable UU Aur. 06 36.7 -22 37 H 60 H II 60. 06 36.8 +41 08 STF 933 Proper motion of B -005 +006. 06 37.1 +24 44 POU 1650 Position corrected. 06 37.1 +24 21 POU 1649 Position corrected. 06 37.1 +03 12 BAL 2181 Proper motion of B -007 -001. 06 37.6 +12 11 S 529 AB: B is BD+12@1221. Proper motion of B -002 -002. 06 37.7 +61 29 STT 8 Lyn. 06 37.7 +16 24 BUP 90 H V 71. Gamma Gem. A is a long-period spectroscopic pair, P = 12.4yr. 06 37.8 +23 11 STF 943 Proper motion of B +095 -049. 06 38.4 +28 59 MCA 27 53 Aur. An occultation and interferometric binary. P = 22.3yr., a = 0.15", motion retrograde. 06 38.6 +40 20 FRK 6 Proper motion of B -002 -017. 06 38.6 -48 13 DUN 31 B is CD-48@2416. A is variable. Proper motion of B +138 -141. 06 38.8 -22 55 BRT 1392 CD-22@3315. 06 39.1 +02 20 AG 118 Proper motion of B -016 -004. 06 39.3 +42 29 BUP 92 Psi (3) Aur. 06 39.3 +42 00 STT 150 Often too close to measure. Rapid binary. 06 39.3 +31 35 S 528 A is an Algol-type system, AK Aur. 06 39.6 +28 16 STT 152 54 Aur. A is a spectroscopic binary. 06 39.6 -23 42 FIN 321 Few measures, which leave the nature of the motion uncertain. 06 40.1 -30 33 COO 40 Proper motion of B -040 +004. 06 40.2 +33 42 GYL 80 Proper motion of B -046 -007. 06 40.5 +00 57 BAL 1322 Proper motion of B +001 -006. 06 41.0 +09 54 STF 950 A is an irregular variable, S Mon. A measure of STF 950 A and D 11 C. A measure of STF 950 A and STF 952 A. E is BD+10@1223. F is BD+09@1338. Proper motion of F -002 -001. 06 41.2 +09 28 STF 954 Spectrum of B: B9V. 06 41.2 +08 59 STF 953 Proper motion of B -011 -001. 06 41.2 -07 59 STF 955 Proper motion of B -007 +014. Proper motion of C 000 +010. 06 41.3 +28 12 HJ 397 25 Gem. 06 41.5 +09 50 STF 3118 BDS 3565 probably same star. 06 41.8 +30 41 A 218 P = 86yr., a = 0.27", motion retrograde. 06 42.3 -22 50 BRT 1393 CD-22@3396. 06 42.3 -38 24 DUN 32 Proper motion of B +047 -010. 06 42.5 +66 12 MLR 318 A premature orbit has been calculated. 06 42.7 -21 55 B 2121 CPD-21@1431. 06 42.8 -40 51 I 1156 I 1156 1/2. 06 42.8 -50 27 HJ 3889 B is CD-50@2356. 06 43.8 +03 27 A 2824 Proper motion of B -013 +008. 06 43.9 +25 08 S 533 Epsilon Gem. B is BD+25@1407. Proper motion of B -006 -010. 06 44.0 +13 14 LAM 3 30 Gem. 06 44.0 +07 29 J 666 There is a 14th magnitude star 8" np C. 06 44.2 -54 42 DUN 34 B is CPD-54@1096. 06 44.3 +40 37 STT 154 B is BD+40@1697. Proper motion of B 000 -018. 06 44.5 -31 04 HDO 197 10 CMa. A is the variable FT CMa. 06 44.9 +07 28 J 2009 Proper motion of B -015 -004. 06 45.0 +13 46 STF 959 Proper motion of B -012 -010. 06 45.1 -16 43 AGC 1 AB: Sirius. Magnitude of A -1.58. Proper motion of A -553 -1205. P = 50.1yr., a = 7.50", motion retrograde. BC: Suspected by Fox in 1920, also reported by Innes, van den Bos, and Finsen. Oother observers fail to confirm duplicity of B. Single 1945, 1946, 1949, 1950. 06 45.2 -35 12 RST 5247 Spectrum: A2/3(m)F0-F2/3. 06 45.5 +49 24 HU 564 Round 1944-1954 with 82-inch. 06 45.5 +29 22 A 122 A premature orbit has been computed. 06 45.5 -30 57 HJ 3891 This is the variable HP CMa. 06 45.6 +54 20 A 1735 Rapid retrograde motion, but few measures. 06 45.6 +02 19 BAL 1717 Proper motion of B +007 +008. 06 45.7 -20 41 HJ 2341 B is BD-20@1548. Proper motion of B -019 000. 06 46.2 +59 27 STF 948 12 Lyn. A premature orbit has been computed. 06 46.2 +12 59 J 2592 Same measure was published as J 2594. 06 46.7 +43 35 SHJ 75 Psi (5) Aur. B is BD+43@1596. 06 46.7 +13 05 J 2437 Not seen by Heintz. May be J 2593. 06 46.7 -47 48 HJ 3895 Proper motion of B +005 +011. 06 46.8 +13 00 J 2593 See JO 27, page 5. 1914.09, 150@, 2.5", 9.5-9.7. 06 47.4 +18 12 STT 156 P = 249yr., a = 0.46", motion retrograde. 06 47.5 -76 51 HJ 3911 B is CPD-76@423. Proper motion of B -026 000. 06 47.8 +00 20 STT 157 P = 299yr., a = 0.56", motion retrograde. 06 47.8 -11 43 STF 970 B is BD-11@1637. Proper motion of B -025 +051. 06 48.1 -09 48 A 1056 A premature orbit has been computed. 06 48.2 +55 42 STF 958 A has variable proper motion. B is a spectroscopic binary. 06 48.2 +26 42 STF 962 Proper motion of B +007 -002. STF 972 BC: Probable rapid motion, but few measures. 06 48.5 +10 10 ARG 64 B is BD+10@1277. 06 48.7 +07 37 A 2731 P = 400yr., a = 0.90", motion direct. 06 49.0 -15 09 AC 4 A is a spectroscopic binary. 06 49.6 +53 02 STF 960 Proper motion of B -001 -058. 06 49.6 -24 09 S 538 Proper motion of B -002 -016. 06 49.8 +16 12 J 2028 33 Gem. This is the variable OV Gem. 06 50.0 +41 00 H 71 H II 71. STF 967 rej. Identification not certain. 06 50.0 -45 27 I 159 Variable. 06 50.3 +24 09 COU 768 P = 22yr., a = 0.18", motion retrograde. 06 50.4 -31 42 H 108 H V 108. B has variable radial velocity. 06 50.8 +41 47 ENG 27 Psi (7) Aur. 06 51.0 -56 14 HJ 3898 B is CPD-56@1180. Proper motion of B -023 +044. 06 51.4 +18 40 STF 976 B is BD+18@1372. Proper motion of B -009 -011. 06 51.5 +54 12 A 1573 Apparently in rapid motion. 06 51.6 +21 46 BU 1193 36 Gem. 06 51.6 -01 21 BAL 349 A is a Cepheid, SZ Mon. 06 51.6 -77 08 HJ 3926 B is CPD-76@426. 06 51.7 +25 03 A 512 P = 187yr., a = 0.21", motion direct. 06 51.7 -44 18 LDS 173 B is CD-44@2973. 06 52.2 -56 31 GLI 50 B is CPD-56@1185. Common proper motion -007 -056. B is a Beta Lyrae-type system. 06 52.8 +33 58 FOX 150 Theta Gem. A is a spectroscopic binary. 06 52.8 +24 58 A 513 P = 347yr., a = 0.67", motion retrograde. AC: See ADS for differences in R.A. and Dec. 06 52.9 +52 41 STF 968 Proper motion of B +000 -011. 06 53.0 +38 52 STF 974 59 Aur. A is a Delta Scuti-type variable, OX Aur. 06 53.0 -26 57 SEE 71 A is variable. 06 53.1 +59 27 STF 963 14 Lyn. P = 335yr., a = 0.63", motion direct. 06 53.2 +38 26 COU 1877 60 Aur. 06 53.2 -00 13 J 1057 1896 measures of 2 additional companions are given in Ann. de l'Observatoire de Besancon Vol. III. 06 53.3 +57 50 A 1321 Not seen in 1944. Round 1950. Fairly rapid motion. 06 53.5 +51 39 ES 2620 B is BD+51@1248. Proper motion of B +005 -014. 06 53.5 +39 51 A 3039 Not seen since discovery, possbly due to an incorrect right ascension. 06 53.6 -20 49 BRT 306 CPD-20@1733. 06 53.7 +23 33 DOO 37 This star is not HJ 401. See HJ 401 at 06 54.0,+23 19 (Doolittle). 06 53.9 -04 24 STF 985 B is BD-04@1713. Proper motion of B +012 -004. 06 54.0 +23 19 HJ 401 See star at 06 53.7,+23 33, BD+23@1527. Doolittle identifies both stars. 06 54.0 -10 02 STF 988 B is BD-09@1714. Proper motion of B -006 +001. 06 54.1 +60 52 HEI 334 L1815-5. Long-period astrometric binary now resolved. P = 12yr., a = 0.34", motion retrograde. Very sparse visual data. 06 54.1 +06 41 STT 79 B is BD+06@1428. Proper motion of B 000 +001. 06 54.2 +66 50 MLB 1068 Proper motion of B -004 -009. A faint star almost exactly between A and B. 06 54.5 -27 34 B 706 P = 1462yr., a = 1.93", motion direct. 06 54.6 +13 11 STF 982 38 Gem. A is a Delta Scuti-type variable. A premature orbit has been computed for AB. 06 54.6 +02 37 AG 124 Proper motion of B +002 -035. 06 54.8 +03 34 STF 989 Proper motion of B -018 -019. 06 54.8 -74 17 HJ 3927 B is CPD-74@423. Proper motion of B -022 -003. 06 55.0 -20 24 H 65 H V 65. 17 CMa. B is BD-20@1625. Proper motion of B +004 -004. 06 55.1 +32 08 BUP 94 Nova Gem. No. 2, DN Gem. 06 55.2 +08 16 J 2034 May be same star as J 274. 06 55.5 +02 34 AG 125 Proper motion of B -009 -014. 06 55.6 -13 59 GAL 278 Possibly BD-13@1732. 06 55.6 -20 08 H 123 H N 123. Pi CMa. Possibly variable. 06 55.8 -11 52 STF 993 B is BD-11@1695. Proper motion of B +007 -040. 06 55.9 -31 47 JSP 125 A is a spectroscopic binary. 06 56.1 -14 03 STF 997 Mu CMa. 06 56.6 +28 58 HJ 742 Proper motion of B -015 -016. 06 56.6 -22 39 S 541 B is BD-22@1610. Proper motion of B +012 +014. 06 57.1 -01 08 BAL 743 Proper motion of B -008 -030. 06 57.3 +58 25 STT 159 15 Lyn. P = 210yr., a = 1.03", motion direct. 06 57.3 -35 30 I 65 P = 16.7yr., a = 0.22", motion direct. 06 57.3 -49 29 RST 5253 A premature orbit has been computed. 06 57.5 +02 53 A 2681 Ambiguous case: P = 250 or 85yr., a = 0.27 or 0.18", motion retrograde. 06 57.5 -19 49 HDO 93 CPD-19@1581+2. 06 57.9 -44 17 LPM 248 Proper motion -1129 -119. 06 58.5 -11 26 STF 1004 Proper motion of B -006 -006. 06 58.6 +06 41 J 278 ADS gives BD as +06@1463. 06 58.6 -00 16 RST 5252 Measures formerly attributed to A 1737 apparently belong to this pair. 06 58.6 -25 25 B 124 A is a spectroscopic binary. 06 58.6 -28 58 CPO 7 Epsilon CMa. 06 58.7 -31 00 HDO 198 Proper motion of B -005 -001. 06 58.8 +26 05 CHR 170 39 Gem. 06 59.5 +37 06 STF 994 Companions D and E not found in photographic catalogue. Proper motion of B +001 -004. 06 59.5 +25 55 MCA 28 40 Gem. 07 00.2 -22 43 S 543 B is BD-22@1642. 07 00.3 -22 07 FIN 334 A variable, FU CMa. 07 00.4 +12 27 BRT 2285 Declination corrected by Heintz. 07 00.5 +02 39 AG 131 Proper motion of B +007 -013. 07 00.5 -00 31 BAL 749 Proper motion of B -019 -028. 07 00.5 -60 52 HJ 3924 B is CPD-60@743. 07 00.6 +09 21 KU 92 Proper motion of B -006 -009. 07 00.7 +45 27 ES 1324 Proper motion of B -018 -040. 07 00.8 +31 56 AG 129 Proper motion of B -010 +016. 07 00.8 +27 16 BU 1022 Round 1952-1956. 07 01.2 +11 46 STT 163 A premature orbit has been calculated. 07 01.3 +52 03 HJ 2354 ES 1078. Probably an error in HJ's angle (ADS). 07 01.3 -52 42 BRT 2024 CD-52@1784. 07 01.5 -09 42 A 3042 P = 118yr., a = 0.25", motion direct. 07 01.6 +39 50 AG 130 Proper motion of B -002 +007. 07 01.6 +02 33 AG 133 Proper motion of B -021 -011. 07 01.7 -27 56 B 126 Sigma CMa. An irregular variable. 07 01.8 -11 18 HU 112 A variable, GU CMa. 07 01.9 -01 21 KUI 28 Proper motion of B 000 -019. 07 02.1 -06 37 J 359 Declination was 15' in error, according to Heintz. 07 02.3 +12 35 HJ 3288 B is BD+12@1394. Proper motion of B -006 -006. 07 02.6 +15 58 A 2462 Ambiguous case: P = 44 or 95yr., a = 0.20 or 0.25", motion retrograde. 07 03.1 +54 10 STF 1001 Proper motion of B -026 -002. 07 03.4 -29 48 HJ 2361 B is CD-29@3827. 07 03.6 +39 41 A 1959 P = 32.6yr., a = 0.24", motion direct. 07 04.0 -43 37 DUN 38 A is a spectroscopic binary. B is CD-43@2907. Proper motion of B -098 +383. 07 04.1 +75 14 STF 973 Proper motion of B -096 -250. 07 04.1 +20 34 SHJ 77 Zeta Gem. A is a Cepheid, and an occultation double. 07 04.2 +56 26 A 1324 Proper motion of B +003 -013. 07 04.2 +49 57 ES 900 Proper motion of B -010 -007. 07 04.3 +01 29 STT 82 B is BD+01@1663. Proper motion of B 000 -011. 07 04.3 -03 03 A 519 P = 42.2yr., a = 0.27", motion retrograde. The A component is a spectroscopic binary, P = 5.72d. 07 04.5 +41 37 ES 1631 Proper motion of B -013 -003. 07 04.5 -42 32 DON 159 CPD-42@1197. 07 04.7 +05 56 HJ 2360 Proper motion of B -007 -003. 07 04.9 +72 40 STF 980 Proper motion of B -006 -047. 07 04.9 +28 07 STF 1012 Proper motion of B +074 -102. 07 05.1 -47 11 RST 232 CPD-46@1205. 07 05.8 -10 40 D 12 A is a Beta CMa-type variable, V569 Mon. Spectrum; B0.5V+F5III. 07 06.2 +04 25 J 2452 J 2608 probably same star. 07 06.5 -01 34 BAL 399 B of BAL 399 is A of BAL 400. 07 06.5 -01 34 BAL 397 B of BAL 397 is also B of BAL 400. 07 06.7 -11 18 BU 328 A is the Beta CMa-type variable, FN CMa. 07 06.9 +62 33 STF 1006 B is BD+62@904. Proper motion of B -019 -009. 07 07.2 +16 50 STF 1017 Proper motion of B -004 -021. 07 07.4 +22 42 BLL 19 A is the Mira-type variable, R Gem. 07 07.5 -01 12 CHE 83 Star place uncertain; no BD star near. 07 07.6 -26 16 BRT 2885 CPD-26@1775. 07 07.9 -15 42 A 3043 P = 96yr., a = 0.42", motion direct. 07 08.1 +73 41 PRZ 7 Proper motion of B +013 -011. 07 08.2 +03 23 HJ 2362 B is BD+03@1561. 07 08.4 +15 56 STT 165 45 Gem. B and C are optical. 07 08.4 -26 24 BU 1412 Delta CMa. 07 08.5 +24 59 STF 1023 B is BD+25@1585. Proper motion of B +003 -011. 07 08.7 -70 30 DUN 42 Gamma (2) and Gamma (1) Vol. B is a spectroscopic binary and is variable. Proper motion of B +028 +096. 07 08.8 +35 54 STF 1018 Proper motion of B -015 -015. 07 08.8 +16 55 STF 1027 Proper motion of B -003 +008. 07 08.8 -08 41 STF 1030 Proper motion of B -004 -012. 07 09.0 +01 14 FOX 152 Proper motion of B -004 -009. 07 09.1 -26 55 B 710 CPD-26@1815. 07 09.2 -56 22 DUN 40 B is CPD-56@1262. Proper motion of B -011 +004. 07 09.3 +03 26 BAL 2250 BAL suspected A to be double. 07 09.3 -49 59 HJ 3935 B is CD-49@2647. 07 09.6 +25 44 HO 519 A is a spectroscopic binary, P = 32.81d. 07 09.7 -25 14 B 2136 A spectroscopic binary. One component variable? 07 09.9 +58 06 HJ 2359 Proper motion of B -001 +007. 07 10.2 -04 14 BUP 97 20 Mon. 07 10.2 -18 41 RST 2456 HR 2705. 07 10.3 -00 51 RST 4839 Proper motion of B -003 -003. 07 10.3 -22 41 DON 167 CD-22@4116. 07 10.4 -55 36 RMK 5 Spectrum: G8/K0III+G/K. 07 11.1 +49 54 ES 2622 Proper motion of B +012 -012. 07 11.1 +30 15 BU 1009 Tau Gem. A is an irregular variable. 07 11.4 -00 25 A 1961 One component is a Delta Scuti-type variable. 07 11.9 -00 30 J 58 Delta Mon. 07 12.0 +22 17 STF 1035 Proper motion of B +042 -037. 07 12.4 -21 58 BRT 1399 CPD-21@1867. 07 12.4 -36 33 BU 757 B may be variable. 07 12.8 +55 48 STF 1025 Proper motion of B +009 -034. 07 12.8 +27 13 STF 1037 P = 116.5 yr., a = 0.93", motion retrograde. Variable? 07 13.1 -01 41 ARG 65 Proper motion of B =001 -010. 07 13.2 -30 58 HJ 3940 This is the variable HO CMa. 07 13.4 +16 10 H 74 AB: H VI 74. 51 Geminorum. A is the semiregular variable variable BQ Gem. 07 13.5 -44 38 HJ 3943 A is a long-period variable. 07 13.7 -20 05 FOX 12 FOX 12a. 07 13.8 -22 54 HJ 3938 B is BD-22@1760. 07 14.2 +04 12 STF 1048 Proper motion of B 000 -006. 07 14.3 -26 21 FIN 323 27 CMa. B is an irregular variable, EW CMa. 07 14.6 -10 18 STF 1052 B is BD-10@1935. Proper motion of B -017 -001. 07 14.7 +24 53 HO 343 52 Gem. 07 14.8 -15 29 BU 575 A premature orbit has been computed. 07 15.3 -00 10 BU 1268 24 Mon. 07 15.6 -63 11 R 72 B is CPD-62@805. 07 16.0 -29 30 HJ 2370 B is CD-29@4143. Proper motion of B +001 -007. 07 16.1 +02 02 BAL 1783 Proper motion of B -016 +002. 07 16.6 -23 19 HJ 3945 B is CD-23@5192. Proper motion of B -032 +037. 07 16.6 -51 00 HJ 3951 A is a semi-regular variable. 07 16.8 +00 59 A 2855 P = 66yr., a = 0.34", motion retrograde. 07 17.0 -30 54 BSO 2 B is CD-30@4233. Proper motion of B +001 -018. 07 17.1 -12 02 A 2123 P = 131yr., a = 0.25", motion direct. C is physical. 07 17.1 -37 06 DUN 43 Pi Pup. B is CD-36@3487. Proper motion of B -014 +005. 07 17.2 -23 51 I 773 ADS 5960a. 07 17.5 -46 59 I 7 P = 82yr., a = 0.56", motion retrograde. 07 17.6 +09 18 STT 170 A premature orbit has been computed. Speckle would be useful as the pair closes in. 07 18.1 +34 57 STF 1054 Proper motion of B +013 -027. 07 18.1 +16 32 STF 1061 Lambda Gem. A is a spectroscopic and occultation binary, and may be variable. 07 18.1 +04 21 STF 1063 J 1992. BAL 2753. Proper motion of B -022 -008. Proper motion of C -018 -014. 07 18.1 -13 42 STF 1069 B is BD-13@1925. Proper motion of B +005 +009. 07 18.3 -36 44 JC 10 A is the variable NV Pup. Spectrum composite; B2V+B3IVne. B is NW Pup. 07 18.7 -24 57 FIN 313 Tau CMa. A is a Beta Lyrae-type system and probably variable. 07 18.8 +02 52 STF 1067 Proper motion of B -015 -014. 07 18.8 -24 49 BRT 2893 CPD-24@2231. 07 19.0 +22 43 HJ 416 Proper motion of B -018 -007. 07 19.2 -24 57 B 133 Variable radial velocity. 07 19.3 -22 03 LAL 53 Proper motion of B -017 -011. 07 19.3 -24 53 B 134 CPD-24@2250. 07 19.9 +54 55 STF 1050 Proper motion of B +002 -027. 07 20.1 +21 59 STF 1066 Delta Gem. A premature orbit has been computed. A is an occultation double, and a long-period spectroscopic binary. 07 20.1 +01 46 AG 138 Proper motion of B -013 +002. 07 20.1 -21 53 I 391 D is CPD-21@2035. 07 20.4 -52 19 RMK 6 Spectrum of B G0V:e. Proper motion of B -078 +147. 07 20.5 +68 32 STF 1038 Proper motion of B +001 -029. 07 20.6 -01 36 A 1963 Rapid binary. Too close 1957 with 82-inch. Needs speckle. 07 20.7 -52 12 HJ 3958 B is CD-51@2444. Proper motion of B +024 -025. 07 20.7 -62 05 JSP 158 Spectral type G0? 07 20.8 +31 28 S 546 B is BD+31@1541. Proper motion of B +009 -018. 07 20.9 -26 58 SEE 76 A is a variable, HQ CMa. 07 21.0 -21 57 BRT 315 CPD-21@2062. 07 21.4 -48 32 DUN 45 B is CD-48@2891. Proper motion of B -003 +023. 07 21.7 -61 57 BSO 16 A is the variable V389 Car. B is CPD-61@813, proper motion +017 +023. 07 21.9 +46 14 ES 2624 B is BD+46@1254. Proper motion of B -001 -014. 07 21.9 +20 27 BU 1413 56 Gem. A is a suspected variable. 07 22.0 +36 46 BU 901 65 Aur. 07 22.2 -24 12 HJ 5451 HJ 5451a. 07 22.3 +59 54 STF 1055 47 Cam. 07 22.3 +50 09 STF 1065 20 Lyn. Spectroscopic binary. Proper motion of B -031 -036. 07 22.3 +04 29 STF 1080 Proper motion of B +003 -018. 07 22.3 -35 55 HJ 3957 Proper motion of B -018 +116. 07 22.9 +55 17 STF 1062 19 Lyn. Both components appear to be spectroscopic binaries. 07 23.0 +45 00 STF 1071 Proper motion of B -014 +005. 07 23.0 -25 46 B 719 VY CMa. This multiple "star" is involved in nebulosity, shaped like the tail of a comet. All companions may be knots in the nebulosity, and all may seem variable. 07 23.8 +10 42 STF 1082 Proper motion of B -005 -006. 07 24.1 -29 18 SMY 2 Eta CMa. B is CD-29@4321. Proper motion of B -007 -003. 07 24.2 -26 37 RST 1345 CPD-26@2080. 07 24.6 +37 49 STF 1079 C of STF 1079 is A of BU 1414 (07244+3746). 07 24.7 -31 49 DAW 129 A is a suspected variable. 07 24.8 -37 17 HJ 3966 Proper motion of B -062 +082. 07 25.0 -38 21 LDS 180 B is CD-38@3367. Proper motion of B -023 -111. 07 25.2 -05 44 SCJ 5 B is BD-05@2105. 07 26.0 +14 06 STF 1088 Proper motion of B -007 -014. 07 26.2 +37 49 ALI 834 Two recent observations show this object to be single. 07 26.2 +14 50 STF 1089 Proper motion of B -004 -034. 07 26.5 +18 31 STF 1090 Proper motion of B -020 -021. 07 26.5 -39 37 WG 62 May be CD-39@3313. 07 26.9 +20 15 CHR 26 61 Gem. An occultation and spectroscopic binary, now resolved. 07 27.0 -34 19 HJ 3969 B is CD-34@3610. Proper motion of B -312 +093. 07 27.2 +08 17 BUP 101 Beta CMi. A is a spectroscopic binary. Variable? 07 27.4 +08 45 STF 1095 Proper motion of B 000 +013. 07 27.5 -20 47 ARG 17 B is BD-20@1949. 07 27.6 -18 30 S 550 B is BD-18@1847. Proper motion of B +004 +002, spectral type B8I. 07 27.7 +63 00 STF 1075 Proper motion of B 000 -016. 07 27.7 +21 27 MCA 30 63 Gem. A is a spectroscopic binary and occultation triple, with the wider pair, presumably, now resolved. 07 27.9 +04 48 BAL 3007 BAL claimed A had a closer companion. 07 27.9 -11 33 BU 332 Spectrum: G8Ib-II+B+B8V. Proper motion of B -009 000. Variable? 07 28.0 +06 57 BU 21 Eta CMi. 07 28.2 +08 56 LAM 4 Gamma CMi. A is a spectroscopic binary. 07 28.2 -20 11 BHA 5 CPD-19@2220. 07 28.5 +36 08 AG 141 Proper motion of B +004 +021. 07 28.7 +24 39 STT 85 B is BD+24@1666. Proper motion of B -019 +014. 07 28.8 -44 32 DON 186 CPD-44@1586. 07 28.9 +48 11 KUI 30 A may be a long-period spectroscopic binary. 07 29.1 +31 47 A 2124 Rho Gem. A is a spectroscopic binary. 07 29.2 +14 21 STT 86 B is BD+14@1676. Proper motion of B -008 -009. 07 29.2 -43 18 DUN 51 Sigma Pup. A is a spectroscopic binary. Proper motion of B -063 +188. 07 29.4 -15 00 STF 1104 AB: Proper motion of B -173 -230. A premature orbit has been computed for AB. 07 29.4 -75 03 HJ 3991 B is CPD-74@444. 07 29.7 -02 42 BAL 173 BAL 172 is a close pair. B of BAL 173. 07 29.8 +27 55 MCA 31 65 Gem. A is a spectroscopic binary, now resolved by speckle interferometry. 07 29.9 +49 40 ENG 31 22 Lyn. 07 30.0 +49 58 STF 1091 Proper motion of B +004 -014. 07 30.1 -45 09 CPO 159 CPD-44@1605. 07 30.3 +49 59 STF 1093 P = 380yr., a = 0.77", motion direct. 07 30.4 +13 52 STF 1102 South measures a 7th magnitude pair: 1825.09, 50.3@, 111.6". Proper motion of B -053 -035. 07 30.8 +04 18 BAL 2771 Baillaud thought A had a closer companion. 07 30.9 +30 34 DOM 1 C is BD+30@1520. 07 31.2 -21 10 BRT 317 CPD-20@2532. 07 31.3 +16 19 STF 1106 Proper motion of B +017 -008. 07 31.7 -35 53 JSP 167 A is a spectroscopic binary and ellipsoidal variable, PS Pup. BC is CPD-35@1289. 07 31.9 +36 13 LDS 6206 Ross 989, VYS 246. Component A is VV Lyn, so designated because of starspots, but later also found to be a flare star. Spectrum of B dM4.5e. 07 32.0 -08 41 STF 1111 Spectrum composite; A+G. Proper motion of B -010 -006. 07 32.2 +14 05 HU 1244 P = 93yr., a = 0.84", motion retrograde. 07 32.5 -38 58 B 1550 Spectrum: A3/5mA7-F2. 07 32.6 -12 53 STF 1115 B is BD-12@2017. 07 32.7 +05 40 ARG 67 B is BD-05@1702. 07 32.8 +22 53 STF 1108 Spectroscopic binary. Spectrum: K0II-III+F8V. Proper motion of B -029 -025. 07 32.8 -49 13 HJ 3981 Proper motion of B -004 +010. 07 33.1 -57 56 LPO 9 Spectral type A2? 07 33.2 +32 52 BU 22 Proper motion of B -013 +005. 07 33.6 +15 50 MCA 32 68 Gem. 07 33.7 +09 17 STF 1114 Proper motion of B -011 +009. 07 33.7 -15 09 A 3091 RST gives magnitudes as 9.2-9.6. 07 34.1 -50 50 HJ 3986 B is CD-50@2840. 07 34.2 -50 45 BRT 713 CPD-50@1299. 07 34.3 +03 22 J 2835 BAL 2296. Delta (3) CMi. 07 34.3 -23 28 H 19 H N 19. A is a spectroscopic binary. Spectrum of B: F5/7V. 07 34.5 -13 52 DOO 42 Slightly variable. 07 34.6 +31 53 STF 1110 Alpha Gem. Castor. Mt. Wilson spectral types A2,A2,M1. P = 467yr., a = 6.80", motion retrograde. A and B are both spectroscopic binaries, and C is the eclipsing binary YY Gem, P =0.81d, so the object is sextuple. Castor A is also reported to exhibit x-ray and radio emission. 07 34.7 +20 10 HJ 2396 Proper motion of B -013 -013. 07 34.8 +59 33 STF 1098 Proper motion of B -014 +011. 07 34.9 -20 10 BRT 320 CPD-19@2360. 07 35.1 +30 58 STT 175 P = 213yr., a = 0.55", motion retrograde in a very highly-inclined and eccentric orbit. 07 35.4 -05 59 SCJ 6 B is BD-05@2176. 07 35.4 -74 17 HJ 3997 A is a spectroscopic binary. 07 35.7 +43 03 MAD 3 Called MA 2 in BDS and ADS. MA 2 is 05214-0653. 07 35.9 +26 54 BUP 103 Upsilon Gem. Variable? 07 36.1 +36 52 ES 2157 Van Biesbroeck measure of BD+37@1743: 1944.29, 223.9@, 1.18", 10.8-11.2. He questions Espin's identification. 07 36.2 -48 51 HJ 3988 Proper motion of B -003 -004. 07 36.3 +00 03 HJ 762 Proper motion of B -013 +013. 07 36.6 -14 29 STF 1121 AB: B is BD-14@2021. Proper motion of B -032 -024. AI: Proper motion of I +008 +005. AJ: Proper motion of J -022 -006. 07 36.7 -14 27 S 555 B is BD-14@2022 (G of STF 1121). Proper motion of B +002 -015. 07 36.8 -15 55 RST 3530 Spectrum: Fm Delta Del. 07 37.3 -04 07 BUP 104 25 Mon. A variable? C is BD-03@1978. 07 37.6 -14 26 S 557 B is BD-14@2052. Proper motion of B -003 -005. 07 37.7 -29 46 LDS 191 Durchmusterung identification doubtful. 07 37.9 -60 26 HJ 3993 CD-60@1821. 07 38.0 -32 08 B 1554 This is the variable PU Pup. Measures by van den Bos and Finsen in 1938 have angles 100 degrees less. 07 38.2 +17 52 HJ 2404 A measure of A and BD+18@1692. 07 38.3 -25 22 B 731 Duplicity still not certain. Needs speckle. 07 38.3 -25 24 I 778 CPD-25@2621. 07 38.4 +36 44 HZG Optical. 07 38.4 +09 58 HJ 763 Proper motion of B -005 -015. 07 38.4 -47 43 HJ 3990 B is CD-47@3192. 07 38.5 +35 03 BU 200 70 Gem. AC: H VI 70. 07 38.8 -26 48 H 27 H III 27. Both components suspected variables. 07 38.9 +42 29 STT 87 B is BD+42@1745. Proper motion of B -015 000. 07 38.9 -20 16 ARG 47 ARG 47a. 07 39.3 +05 14 SHB 1 Alpha CMi. Procyon. P = 40.65yr., a = 4.55", motion direct. Proper motion of A -710 -1023 (FK5). LAM AC: Proper motion of C -003 +001. 07 39.3 -38 26 B 1557 CPD-38@1481. 07 39.4 -43 58 HJ 3992 Proper motion of B -013 -014. 07 39.7 +01 17 A 2532 Rapid motion. 07 39.7 -22 50 BRT 1426 CD-22@4893. 07 39.9 -22 31 BRT 1428 CD-22@4899. 07 40.0 -03 36 BGH B is BD-03@2002. Proper motion of B +065 -282. 07 40.0 -24 53 I 779 CPD-24@2670. 07 40.1 +05 14 STF 1126 One component is a spectroscopic binary. 07 40.2 -17 24 LUY 6207 LUY 745-46A. Listed by Luyten in Ap.J. 112, 213. 07 41.0 +21 48 STF 1124 Proper motion of B -025 -003. 07 41.1 -01 24 A 1968 P = 235yr., a = 0.40", motion retrograde. 07 41.2 +01 08 AG 143 Proper motion of B -010 -016. 07 41.4 +01 49 KU 93 Proper motion of B -013 -022. 07 41.4 -85 55 HJ 4086 B is CPD-85@138. 07 41.6 +09 12 SCJ 7 Proper motion of B -007 -001. 07 41.7 +37 26 STT 177 P = 165yr., a = 0.33", motion retrograde. 07 41.7 +09 42 STF 1130 A premature orbit has been computed. Needs speckle. 07 41.8 -72 36 DUN 57 Zeta Vol. Proper motion of B +036 +019. 07 42.1 -24 07 CPD 4 B is CD-23@5971. 07 42.2 -03 31 STF 1132 B is BD-03@2018. Proper motion of B -012 -011. 07 42.9 +65 17 HEI 132 HU 843 is identical, misidentified by Hussey (Heintz). 07 43.0 +58 43 HJ 2405 24 Lyn. 07 43.0 +23 27 BLL 22 A is the Mira-type variable, S Gem. 07 43.0 -17 04 HU 710 P = 138yr., a = 0.35", motion retrograde. 07 43.1 +00 11 B 2526 Too close or round 1953-1960. Needs speckle. 07 43.3 +28 53 BLL 23 Sigma Gem. A is a spectroscopic binary and variable. 07 43.5 +03 29 STF 1134 Proper motion of B +021 -086. 07 43.5 -28 25 SEE 85 1 Pup. 07 43.7 -37 06 JSP 179 CPD-36@1566. 07 43.8 -39 52 GLI 71 Proper motion of B -007 +001. 07 43.9 +77 53 STF 1100 Schiller measures: 1911.50, 238.6@, 33.54", 8.8-10.5. Identification uncertain. 07 44.2 +49 34 ES 1082 Proper motion of B +027 -028. 07 44.2 -24 57 CPD 5 Proper motion of B +005 +102. 07 44.2 -50 27 DUN 55 B is CD-50@2948. Proper motion of B -112 +140. 07 44.4 +24 24 STT 179 Kappa Gem. 07 44.5 -23 50 BRT 2917 CPD-23@2752. 07 44.5 -23 51 ARA 2067 This, and ARA 2068 may be more distant companions of I 780. 07 44.8 -33 44 STN 60 STN 60 1/2. 07 45.1 -42 48 CPO 169 CPD-42@1599. 07 45.3 +28 02 BU 580 Beta Gem. Pollux. H 42 AC: H VI 42. STF 5 F is BD+28@1465. 07 45.5 -14 41 STF 1138 2 Pup. B is the eclipsing binary PV Pup, and is BD-14@2193. Proper motion -009 -034. 07 45.7 -17 20 POC 1 This is identified by Fenner as AG Washington 2929. 07 45.9 +65 09 STF 1122 BDS 4203, H V 135 same star. Proper motion of B -015 -06 -085. 07 46.1 +21 07 HO 247 P = 250yr., a = 0.47", motion direct. 07 46.2 -30 53 I 1169 Spectrum: Fm Delta Del. 07 46.2 -59 49 COO 58 B is CPD-59@898. Proper motion of B -055 +153. 07 46.5 -22 02 B 2153 CPD-21@2740. 07 46.6 +45 56 ES 587 Proper motion of B -017 -001. 07 47.0 +64 03 STF 1127 BDS 4378; H II 101 is probably same star. 07 47.0 +26 43 BUP 105 Proper motion of D -018 -009. 07 47.0 +00 01 STF 1141 B is BD+00@2080. Proper motion of B -001 -003. 07 47.1 -19 33 DAW 182 CPD-19@2666. 07 47.1 -41 30 DUN 56 Alternate spectral type: B1V. B is CD -41@3385. Proper motion of B -013 +007. 07 47.2 -59 05 R 79 B is CPD-58@993. Proper motion of B -006 +005. 07 47.3 -05 43 HJ 62 There is a faint star near B about half the distance of A. 07 47.5 +33 25 STF 1135 Pi Gem. Variable? 07 47.8 -16 01 KNT 4 B is BD-15@2049. Proper motion of B -001 +001. 07 47.8 -44 18 BRT 716 CPD-43@1790. 07 47.9 -12 12 STF 1146 5 Pup. 07 48.0 +60 18 HU 1247 P = 18.76yr., a = 0.224", motion retrograde. 07 48.1 +05 25 STF 1143 Some error in position. See note in BDS II. 07 48.1 -25 56 SEE 86 Omicron Pup. A is probably variable. 07 48.4 -19 22 OL 5 This is probably the same as OL 156. 07 48.4 -45 15 HJ 4006 Proper motion of B +008 +020. 07 48.5 +28 46 S 560 Proper motion of B 000 -015. 07 48.6 +23 08 WRH 15 82 Gem. 07 48.6 -63 41 HJ 4014 Proper motion of B -012 +023. 07 48.8 +28 55 H 67 H V 67. 07 48.9 -26 22 BRT 2921 CPD-26@2613. 07 49.0 +00 40 STT 88 B is BD+01@1912. Proper motion of B +003 -005. 07 49.1 -56 25 SEE 88 A is a spectroscopic binary. 07 49.2 +37 06 STF 1139 Proper motion of B +042 -020. 07 49.2 +06 05 HJ 61 Proper motion of B +009 -039. 07 49.2 -46 22 JC 11 B is CD-46@3462. Proper motion of B -007 +001. 07 49.3 -24 52 BU 1063 Xi Pup. A is a spectroscopic binary. 07 49.4 -29 02 B 2638 CD-28@4920? 07 49.5 +03 13 STF 1149 Proper motion of B +001 -018. 07 50.0 -02 16 HO 37 Baize notes a couple in the same field to the north, 310@, 8". 07 50.2 -00 53 SAN 1 Reported by Sanford in PASP 52, 408. Star 17 Algiers 184. 07 50.4 -32 10 HJ 4009 Proper motion of B -010 -011. 07 50.6 +20 01 HJ 2418 Proper motion of B -011 -007. 07 50.6 -36 20 JSP 194 CPD-36@1702. 07 50.8 +03 17 A 2880 P = 102yr., a = 0.16", motion direct. 07 51.0 +31 37 STT 89 B is BD+31@1677, spectrum A5. Proper motion of B -012 -044. 07 51.8 -13 54 BU 101 9 Pup. P = 23.2yr., a = 0.57", motion direct. 07 52.5 -13 52 H 28 H III 28. 07 52.6 +12 01 STF 1153 Spectral classes may be F8, F5 (McCormick). B is BD+12@1699. Proper motion of B 000 -013. 07 52.8 -05 26 FIN 325 P = 31.4yr., a = 0.326", motion direct. 07 52.9 +64 54 STF 1136 Proper motion of B +042 -006. 07 52.9 -58 38 RST 4379 Spectral type A5? 07 53.0 +31 38 SEI 483 KU, Bonn 3465. Proper motion of B -013 -031. 07 53.1 +09 06 AG 145 Proper motion of B -001 -015. 07 53.4 +20 50 HJ 432 Proper motion of B -018 +005. 07 53.6 +30 36 BUP 108 Proper motion of A +719 -1832. 07 54.0 +14 57 WEI 17 Proper motion of B -016 -005. 07 54.0 -02 22 BAL 190 Proper motion of B +002 -019. 07 54.2 +04 29 J 803 J notes a second component at 100@, 11th magnitude. 07 54.4 -17 48 HJ 4015 B is BD-17@2221. 07 54.6 -26 41 BRT 2931 CD-26@5181? 07 55.2 +41 34 WEI 16 Proper motion of B -023 +002. 07 55.4 -53 37 GLI 77 B is CPD-53@1479. Proper motion of B +017 -002. 07 55.7 -03 28 HJ 71 See note in BDS II. 07 56.0 +23 42 COU 929 P = 46yr., a =0.18", motion direct. 07 56.0 -23 13 DON 212 CD-22@5380. 07 56.0 -35 55 LPO 12 Proper motion of B -009 +001. 07 56.3 -22 21 SEE 90 CD-22@5387. 07 56.8 -60 49 HJ 4027 In the cluster NGC 2516. Spectra B9IVp(Si) and B9.5IVp(SiII). Spectrum of C: A2IV. 07 57.2 +23 42 HJ 433 Also reported as new by Gauchet and Doolittle. 07 57.3 +01 08 STT 185 P = 59.4yr., a = 0.51", motion direct. 07 57.3 -44 07 SEE 92 A is variable. 07 57.4 +13 12 STF 1162 Proper motion of B -015 -019. 07 57.8 -60 18 LDS 198 A is a spectroscopic binary. JSP 208 BC: CD-59@1774. 07 58.1 -29 16 BRT 2933 CPD-28@2627. 07 58.2 -49 15 HRG 137 A is the Beta Lyrae-type system V Pup. 07 58.3 +02 13 SHJ 87 14 CMi. 07 58.4 -60 51 HJ 4031 Spectrum: B8.5IIIMnII and B9V. Proper motion of B -013 +044. 07 58.7 -47 40 CPO 184 CPD-47@1729. 07 59.0 -63 38 LDS 199 Separation 1050". 07 59.2 -49 59 DUN 59 B is CD-49@3244. Proper motion of B -016 +018. 08 00.8 -47 49 HJ 4033 Proper motion of B -005 -001. 08 01.0 +36 53 HJ 3305 Proper motion of B -030 -014. 08 01.4 +16 57 STF 1173 Proper motion of B -028 -010. 08 01.4 -54 31 DUN 60 One component is variable and a spectroscopic binary. Proper motion of B -002 +004. 08 01.6 -34 30 JSP 216 CPD-34@1901. 08 01.7 +60 19 MCA 33 53 Cam. A variable of the Alpha CVn type, AX Cam, and a spectroscopic binary now resolved by interferometry. P = 6.64yr., a = 0.055", motion direct. 08 01.7 +25 05 H 75 H VI 75. Omega (2) Cnc. 08 01.7 -08 36 A 1580 A is the Algol-type system BV 1594. A rather uncertain visual orbit has been computed: P = 300yr., a = 0.34", motion direct. 08 02.4 +04 09 STF 1175 A premature orbit has been computed. 08 02.5 +63 05 SHJ 86 B is BD+63@750. Proper motion of B +015 +004. 08 02.5 -44 40 I 8 QQ Pup. 08 02.5 -55 02 HJ 4044 B is CPD-54@1480. 08 02.6 +20 28 DOO 47 Doolittle identifies this as BDS 4392, HJ 437 but it seems to be a different pair. 08 02.7 -41 19 HJ 4038 A variable? B is CD-40@3775. Proper motion of B -002 -013. 08 03.1 -06 25 A 1581 A premature orbit has been computed. 08 03.1 -32 28 HJ 4035 B is CD-32@4768. Proper motion of B 000 +001. 08 03.5 +27 48 ES 2628 Chi Gem. See Monthly Notices R.A.S. 68, 205. 08 03.7 -46 34 HJ 4043 B is CD-46@3727. 08 03.9 -31 33 LDS 201 AB: B is CD-31@5466. Proper motion of B -103 +147. AC: C is CPD-31@2104. 08 04.1 +33 02 STT 187 P = 217yr., a = 0.28", motion retrograde. 08 04.4 +12 17 BU 581 P = 44.8yr., a = 0.45", motion direct. C is physical. 08 04.7 +12 04 STF 1179 Proper motion of B -007 -032. 08 04.7 -62 50 DUN 62 A is the variable V375 Car. B is CPD-62@952. Proper motion of B +008 -052. 08 05.0 +58 25 A 1073 P = 119yr., a = 0.25", motion retrograde. 08 05.2 -45 25 JC 12 B is CD-45@3742. Proper motion of B +012 -011. 08 05.4 +08 12 STF 1181 Proper motion of B -009 -013. 08 05.5 +76 48 STF 1151 Proper motion of B -019 -066. 08 05.6 +28 30 MLB 566 The Barton pair formerly at 08049 is identical. 08 05.6 +27 32 STF 1177 Proper motion of B +009 -019. 08 05.6 -66 17 GLI 81 B is CPD-65@867. 08 05.7 -33 34 HJ 4046 Proper motion of B -023 +003. 08 05.9 -01 46 AG 148 Proper motion of B -023 +006. 08 05.9 -20 14 ALD 84 CPD-19@3088. 08 06.1 -00 47 A 1971 A premature orbit has been computed. 08 06.2 +02 01 J 420 Appears to be in rapid retrograde motion. 08 06.8 +33 03 AG 147 Proper motion of B 000 -012. 08 06.9 -27 07 DUN 61 B is CD-26@5531. 08 07.1 -21 38 B 2168 CPD-21@3163. 08 07.2 +07 23 AG 149 Proper motion of B -004 -123. 08 07.4 +00 12 BAL 1132 Proper motion of B +010 -012. 08 07.5 -12 12 A 2749 P = 179yr., a = 0.33", motion direct. 08 07.5 -24 18 RST 5284 Rho Pup. A is a Delta Scuti-type variable. 08 07.9 -01 21 STF 1189 Proper motion of B +006 +001. 08 07.9 -68 37 RMK 7 Epsilon Vol. A is a spectroscopic binary. 08 08.0 +46 11 ES 1144 Proper motion of B -023 -003. 08 08.2 +21 06 COU 91 Proper motion of B -287 -358. 08 08.5 +51 30 ES 70 27 Lyn. 08 08.6 -02 59 STF 1190 Zeta Mon. C is BD-02@2449. Proper motion of C -009 +005. 08 09.1 -37 19 BRT 1615 CPD-36@1978. 08 09.1 -39 31 GLI 80 B is CD-39@4038. Proper motion of B -003 -001. 08 09.4 +37 52 STF 1184 B is BD+38@1869. Proper motion of B +018 +010. 08 09.4 +30 21 STF 1188 Proper motion of B +012 +011. 08 09.5 -47 20 DUN 65 Gamma (2) Vel. B is CD-46@3846, Gamma (1) Vel. Both components are spectroscopic binaries, and B is variable. A is probably the nearest Wolf-Rayet system. Spectrum: WC8+O7.5e. Spectrum of B B1IV. I 1175 DE: DE is I 1175 (= RST 4878) at 08 09.5 -47 25. 08 09.8 -16 58 A 3101 Spectrum: A3/5II/III. 08 10.0 -42 41 CPO 195 CPD-42@2143. 08 10.1 +04 03 AG 150 Proper motion of B +026 +001. 08 10.2 +25 51 BUP 111 B is BD+26@1729. Proper motion of B -104 -048. 08 10.4 +00 20 BAL 1133 Proper motion of B -030 -017. 08 10.5 +25 30 BUP 112 Psi Cnc. Optical. 08 10.7 -13 48 LDS 204 18 Pup. 08 11.2 +32 55 SEI 488 Proper motion of B +010 -014. 08 11.3 +01 17 STF 1198 B is BD+01@2018. Proper motion of B -076 -005. 08 11.3 -12 56 BU 1064 19 Pup. Not seen in 1936, 1939 (van den Bos). 08 11.4 -42 59 HJ 4057 B is CD-42@3976. 08 11.6 -37 22 JSP 236 CPD-37@1984. 08 12.1 -15 40 HJ 4050 B is BD-15@2309, proper motion -009 +009, spectrum A9/F0V. 08 12.2 +17 39 STF 1196 Zeta Cnc. P = 59.7yr., a = 0.88", motion retrograde. AB-C: A premature orbit has been computed. An unseen companion of C with P = 17.2yr. is known. AB-D: D is BD+18@1870. 08 12.2 -01 50 J 421 The note in ADS says that the 1906 measures by Morgan, attributed to HJ 778, may belong to this pair. 08 12.9 +09 35 STF 1201 Proper motion of B -037 -004. 08 13.0 -54 02 HJ 4065 B is CPD-53@1569. 08 13.2 -13 54 HU 115 P = 65yr., a = 0.82", motion direct. 08 13.6 -45 58 COO 69 Proper motion of B +051 +029. 08 13.6 -47 00 GLI 87 A is variable. B is CD-46@3928. Proper motion of B +007 -005. 08 13.7 +04 07 ARG 68 Nys calls B BD+04@1934, instead of A. Proper motion of B -041 +002. 08 13.8 -22 06 LDS 207 CPD-21@3323. 08 14.0 -36 19 DUN 67 Variable, OS Pup. B is CD-35@4360. 08 14.0 -40 21 HJ 4062 The primary is a long-period spectroscopic binary. 08 14.2 +17 41 H 78 H VI 78. 08 14.2 -32 08 HJ 4059 A is a spectroscopic binary. 08 14.3 -31 29 B 1592 Spectrum: A1/2III/IV. 08 14.7 +07 11 STF 1206 Proper motion of B -017 +005. 08 15.3 +05 33 STF 1207 Proper motion of B -006 -006. 08 15.5 -37 22 HJ 4063 B is CD-36@4387. Proper motion of B -068 -005. 08 15.7 +07 38 STF 1209 B is BD+08@2015. Proper motion of B -193 -177. 08 15.8 +02 48 STF 1210 Proper motion of B +004 +003. 08 15.9 +50 47 STF 1199 Opik reverses quadrant. 08 15.9 -30 56 BU 454 Spectrum composite; G5-8III+G:. 08 15.9 -62 52 HJ 4077 B is CPD-62@987. 08 16.0 +49 46 STF 1200 Proper motion of B -016 +009. 08 16.1 -28 47 HLD 95 Spectrum: A2/3III/IV. 08 16.5 +79 30 STF 1169 Proper motion of B -052 -067. 08 16.5 +09 11 BU 1065 Beta Cnc. Burnham measured BD+09@1922 and BD+09@1926 with respect to A (see ADS). A may be variable. 08 17.0 +59 11 STT AB: B is BD+59@1153. Proper motion of B -006 +003. 08 17.3 -05 22 A 337 Ambiguous case: P = 100 or 162yr., a = 0.57 or 0.39", motion retrograde. 08 17.9 +06 28 STF 1213 BDS 4546, HJ 87 probably same star. 08 18.2 -37 22 HJ 4073 A is a spectroscopic binary. 08 18.3 +38 59 STF 1211 P = 407yr., a = 1.11", motion retrograde. 08 18.4 -25 35 B 765 Too close in 1959. Only two measures since discovery. 08 18.6 -42 54 CPO 198 CPD-42@2341. 08 18.7 -34 07 RST 2547 CPD-33@2077. 08 19.4 -38 07 JSP 260 CPD-37@2202. 08 19.5 +35 03 STT 91 B is BD+35@1801. Proper motion of B +078 -138. 08 19.8 -71 31 BSO 17 Kappa (1) and Kappa (2) Vol. A is a spectroscopic binary. 08 20.0 -57 40 CPO 200 B is CPD-57@1483. Proper motion of B -005 +009. 08 20.6 -77 29 I 799 Theta Cha. 08 21.1 +47 25 STT 190 A-CR: AB-CR may be a quadruple system. AD: D is BD+47@1565. Proper motion of D +013 -006. A 1745 CR: P = 280yr., a = 0.48", motion direct. 08 21.2 +04 23 BAL 2815 Proper motion of B -015 -004. 08 21.3 -01 36 STF 1216 P = 254yr., a = 0.52", motion direct. 08 21.4 -35 45 BRT 1623 CPD-35@2261. 08 21.4 -36 29 HJ 4085 A is a spectroscopic binary. 08 21.7 +17 17 PAR A is the Mira-type variable V Cnc. 08 22.1 -73 24 HJ 4103 Eta Vol. 08 22.3 -34 58 BRT 1625 CPD-34@2328. 08 22.5 -29 42 B 1600 Spectrum: Fm Delta Del. 08 22.8 -26 21 B 767 Many negative or uncertain observations. 08 22.8 -76 26 HJ 4109 B is CPD-76@515. 08 23.0 +07 38 STF 1219 Proper motion of B +018 -025. 08 23.1 +20 01 HO 525 P = 122yr., a = 0.44", motion direct. 08 23.3 +68 26 STF 1208 Proper motion of C +016 -005. 08 23.4 -22 07 BRT 1457 CPD-21@3515. 08 23.4 -23 10 BRT 1458 CD-22@6089. 08 23.4 -42 48 HJ 4090 B is CD-42@4188. 08 23.8 +57 25 STT 92 B is BD+57@1136. 08 23.9 +10 38 A 2961 21 Cnc. 08 24.3 +44 57 STF 1217 B is BD+45@1575. Proper motion of B -045 -169. 08 24.4 -46 01 CPO 204 CPD-45@2479. 08 24.5 +34 09 ES 2345 Proper motion of B -034 -007. 08 24.5 -30 39 HJ 2446 B is CD-30@6203. Proper motion of B -077 +023. 08 24.6 -01 09 B 2527 FIN measures 1951-1959 distance less than 0.1". 08 24.7 +42 00 S 565 B is BD+42@1860. 08 24.7 -28 49 RST 1393 A is an Algol-type system, AW Pup. 08 24.8 +64 09 ARG 18 Proper motion of B +008 -007. 08 24.8 +20 09 STT 191 B is BD+20@2078. Proper motion of B -005 -005. 08 25.0 +67 25 LDS 2574 B is BD+67@541. 08 25.1 -49 10 RST 321 P = 25.6yr., a = 0.28", motion direct. 08 25.2 -24 03 S 568 A is a spectroscopic binary. Spectrum composite; K5III+K1III. B is CD-23@7280. 08 25.4 +37 23 HU 856 P = 78.5yr., a = 0.21", motion direct. 08 25.5 -02 07 A 1336 Proper motion of B -021 -004. 08 25.5 -51 44 DUN 69 B is CD-51@3003. Proper motion of B -006 +006. 08 25.6 -53 32 BRT 3286 CD-53@2275. 08 25.9 +07 34 H 109 H VI 109. HJ 785. 08 26.0 -43 18 DON 249 CPD-42@2480. 08 26.3 -39 04 HJ 4093 A is the Algol-type system NO Pup. 08 26.5 +27 54 S 566 Phi (1) Cnc. Proper motion of B -020 -017. 08 26.5 -03 59 H 118 H VI 118. 2 Hya. Possible Delta Scuti-type variable. BDS 4606 is the same star. 08 26.7 +24 32 STF 1224 24 Cnc. Both components suspected of variability. A is physical. A 1746 BC: P = 21.73yr., a = 0.149", motion direct. 08 26.7 -31 55 PRO 59 CPD-31@2369. 08 26.7 -35 31 HJ 4094 Proper motion of B -022 +019. 08 26.8 +26 56 STF 1223 Phi (2) Cnc. Both components suspected of variability. Proper motion of B -007 -008. 08 26.8 -22 52 LDS 219 B is BD-22@2275. Proper motion of B +076 -181. 08 26.9 +32 12 HU 714 P = 123yr., a = 0.41", motion direct. 08 27.0 -52 42 B 1606 P = 14.5yr., a = 0.16", motion direct. 08 27.4 +23 09 STF 1227 Proper motion of B -010 -014. 08 27.6 +62 35 HJ 3309 B is BD+63@799. 08 27.6 -20 51 B 2179 An eclipsing binary, VV Pyx. 08 27.7 +27 34 STF 1228 Proper motion of B -001 -001. 08 27.7 -04 25 A 550 Ambiguous case. P = 43 or 21yr., a = 0.20" or 0.13", motion retrograde. 08 28.0 -35 07 FIN 314 A spectroscopic binary, probably due to motion in the visual pair. 08 28.3 +33 38 SEI 500 Nothing in this position (Heintz). 08 28.4 +16 51 STF 1230 Proper motion of B -002 -035. 08 28.5 -02 31 A 551 P = 54yr., a = 0.28", motion direct, high inclination. Each of the components is itself a spectroscopic binary, and C appears physical, so that the system is quintuple. 08 28.6 +35 02 WOR 19 Possibly ambiguous case, P = 42.1yr., a = 0.20", motion retrograde. 08 28.7 -00 18 BAL 1137 Proper motion of B -004 +006. 08 28.7 -17 32 ARG 20 Proper motion of B -001 -007. 08 28.9 -42 35 HJ 4102 B is CD-42@4287. 08 29.1 -34 56 BRT 1630 CPD-34@2548. 08 29.1 -47 56 FIN 315 One component is a spectroscopic binary. 08 29.5 -44 43 DUN 70 One component is a spectroscopic binary. 08 30.3 +60 43 BU 1067 Omicron UMa. A is variable. 08 30.3 -26 02 B 158 ADS 6847a. 08 30.6 -40 31 DUN 71 B is CD-40@4330. Proper motion of B +010 -022. 08 30.7 +06 26 J 398 Proper motion of B +019 +019. 08 30.7 -43 09 DON 256 CPD-42@2600. 08 31.2 -02 12 BAL 506 Proper motion of B -019 -019. 08 31.3 -19 38 J 1524 Aravamudan gives position 08267-1916 (1900). 08 31.3 -84 41 HJ 4158 B is CPD-84@192. 08 31.4 +31 56 STF 1236 B is BD+32@1747. 08 31.4 -36 42 LDS 223 C is CPD-36@2622. 08 31.4 -39 04 HJ 4107 A is a spectroscopic binary. 08 31.6 +34 58 HU 716 P = 31yr., a = 0.34", motion retrograde. 08 31.6 +18 06 HJ 2452 Theta Cnc. Occultation double. 08 31.8 -03 47 J 416 C was not seen in 1950 (Van Biesbroeck). 08 32.4 -00 56 HJ 96 B is BD-00@2012. Proper motion of B -139 +082. 08 33.0 -49 17 COO 73 Proper motion of B -006 +008. 08 33.1 +55 21 STF 1234 Proper motion of B -006 -033. 08 33.1 -24 36 BU 205 P = 136yr., a = 0.57", motion retrograde. 08 34.4 +07 11 KU 31 Proper motion of B -018 -012. 08 34.4 -44 30 DON 263 CPD-44@2755. 08 34.5 -32 36 FIN 335 P = 17yr., a = 0.16", motion direct. 08 34.5 -37 37 I 195 Variable. 08 35.4 +66 16 STF 1232 B is BD+66@559. Proper motion of B -028 -032. 08 35.8 +06 37 STF 1245 A is a spectroscopic binary. Proper motion of B -134 -137. 08 35.9 +09 55 STF 1246 Proper motion of B -031 -012. 08 36.0 -22 11 B 2182 CPD-21@3748. 08 36.0 -53 37 LPO 70 Spectrum: G2/5(III)+A. 08 36.1 -03 34 LDS 6217 A may be a close double, 50 deg., 2", mag. diff. 0.7. 08 36.2 +13 47 STT 94 B is BD+14@1930. Proper motion of B 000 -001. 08 36.8 +74 43 STT 192 A is a spectroscopic binary. 08 36.9 -30 50 I 68 Spectrum: A3mA7-F2/3. 08 37.5 -53 36 HJ 4123 B is CPD-53@1782. 08 37.7 +19 31 HJ 454 A is a Delta Scuti-type variable. 08 37.7 +05 42 BUP 118 Delta Hya. A spectroscopic binary. 08 37.8 +14 09 HLD 97 Position corrected by Heintz. 08 37.9 -26 15 RST 2571 Eta Pyx. 08 38.4 -46 47 COO 268 Proper motion of B +007 -002. 08 39.1 -22 40 BU 208 CPD-22@3750. P = 123yr., a = 1.70", motion direct, highly inclined. 08 39.1 -70 23 DON 271 Theta Vol. 08 39.4 -36 36 I 314 P = 66yr., a = 0.53", motion retrograde. 08 39.5 -21 00 RST 5506 CPD-20@3936. 08 39.7 +20 05 COU 47 In Praesepe. 08 39.7 -29 34 HJ 4120 Zeta Pyx. B is CD-29@6545. Proper motion of B -019 -091. 08 39.9 +19 33 BU 584 In Praesepe. S 571 C is a spectroscopic binary, and is +20@2153. BU 584 DC: D is variable. Position (2000): 08 39.8 +19 32. In Praesepe. 08 40.0 -53 03 HJ 4126 A is a spectroscopic binary, and is variable. Proper motion of B -027 +019. 08 40.1 +20 00 ENG 37 39 Cnc. A multiple system. A variable? 08 40.1 +20 00 CHR 28 40 Cnc. B of ENG at 08 40.1. In Praesepe. 08 40.1 -35 18 RST 4894 Beta Pyx. A is a spectroscopic binary. 08 40.1 -72 18 GLI 100 Spectrum: G8/K0III+A. 08 40.2 +51 47 STF 1250 Proper motion of B -025 -047. 08 40.3 +19 21 CHR 130 Occultation binary. In Praesepe. 08 40.3 -43 58 CPO 222 CPD-43@2853. 08 40.4 +19 40 STF 1254 D is BD+20@2170. Physical with BD+20@2158. A is a spectroscopic binary. 08 40.4 -42 23 DUN 72 B is CD-41@4370. Proper motion of B +010 -007. 08 40.5 +19 33 S 574 Epsilon Cnc, a spectroscopic binary. B is BD+20@2163. Proper motion of B -030 -015. 08 40.5 -22 55 BRT 1466 CD-22@6471. 08 40.6 -46 39 HJ 4127 Proper motion of B +003 +001. 08 40.6 -59 46 JSP 295 A is a spectroscopic binary and variable, V343 Car. 08 40.7 +35 08 HJ 793 Proper motion of B -018 -025. 08 41.2 -30 05 B 1105 Spectrum: B8/9II/III. 08 41.3 +20 29 BU 585 Spectroscopic binary. In Praesepe. 08 41.4 -47 32 RST 341 CPD-47@2539. 08 41.6 +69 24 PRZ 9 Proper motion of B -032 -073. 08 41.7 +12 11 HJ 2462 Proper motion of B -027 -008. 08 41.7 -15 57 HJ 4124 9 Hya. 08 41.7 -20 18 J 2645 CPD-19@3728. 08 42.0 +62 01 STF 1248 Proper motion of B -045 +026. 08 42.1 -45 43 DON 272 CPD-45@2858. 08 42.1 -52 45 B 1624 P = 76yr., a = 0.40", motion direct. 08 42.1 -62 00 HRG 18 Spectral type F8? 08 42.3 -48 06 RST 5304 A variable, HX Vel. 08 42.4 -53 07 BSO 18 A is a variable, HY Vel. B is CD-52@1605. 08 42.4 -53 07 BSO 18 A is a variable, HY Vel. B is CD-52@1605. B 1625 BC: Position 08 42.3 -53 06. 08 42.5 -08 30 H 107 H VI 107. B is BD-08@2463. 08 43.1 -12 25 RST 3603 P = 85.5yr., a = 0.31", motion retrograde. 08 43.3 +21 28 ENG 38 Gamma Cnc. A is a spectroscopic binary. B is BD+21@1897. 08 43.7 -07 14 S 579 B is BD-06@2707. Proper motion of B -009 -020. 08 43.7 -23 16 BRT 1468 CD-22@6539. 08 43.8 -50 38 BRT 743 CPD-50@1746. 08 43.9 +86 14 STF 1150 Distance uncertain. 08 43.9 +44 03 A 1752 Round 1958 with 82-inch. 08 43.9 +19 02 BLL 26 A is an Algol-type system, S Cnc. 08 44.1 -04 12 A 552 Orbital motion. A difficult pair, < 0.1" in 1953, 1954. 08 44.3 -45 44 DON 277 CPD-45@2933. 08 44.4 -59 57 HJ 4139 B is CPD-59@1097. 08 44.5 +28 27 STF 1266 BDS 4792, H IV 118 same star. Proper motion of B -035 -030. 08 44.7 +18 09 TOK Delta Cnc. Aa-B is optical. 08 44.7 -41 17 I 815 CPD-40@2823. 08 44.7 -54 43 TNG Delta Vel. 08 45.0 +64 30 LDS 2291 Proper motion of B -012 -003. 08 45.2 +41 40 STF 1263 B is BD+42@1923. 08 45.3 +13 16 HJ 105 Proper motion of B -018 -017. 08 45.3 +00 18 HEI 147 Heintz believes Aitken and van den Bos may have observed this pair instead of +00@2380. 08 45.3 -02 36 STF 1270 Proper motion of B -003 +005. 08 46.0 +64 45 H 60 H IV 60. 08 46.1 -46 53 CPO 232 CPD-46@2963. 08 46.2 -14 22 HU 120 P = 216yr., a = 0.50", motion direct. 08 46.4 -13 33 RST 5507 12 Hya. A is a spectroscopic binary. 08 46.6 -42 34 JC 13 Also classed B4V. 08 46.7 +28 46 STF 1268 Iota Cnc. B is CD-29@1823. Proper motion of B -017 -043, spectral type A3V. 08 46.8 +06 25 SP 1 Epsilon Hya. AB: P = 15.05yr., a = 0.255", motion direct. AB is variable. STF 1273 AB-C: P = 890yr., a = 4.54", motion direct. C is a spectroscopic binary, and D is physical. Hence quintuple. 08 47.0 -38 46 B 2186 The nf star of CD-38@4867. 08 47.1 -40 32 WG 114 CPD-40@2867. 08 47.2 +11 10 STF 1276 Proper motion of B -009 -012. 08 47.3 +64 22 MLB 202 Proper motion of B -010 -024. 08 47.4 -41 43 CPO 233 CPD-41@2968. 08 47.6 +00 01 STF 1281 Proper motion of B -010 -037. 08 47.6 -28 22 WNO 3 Proper motion of B -039 -039. 08 47.9 +45 32 ES 596 Proper motion of B -003 -197. 08 48.3 +00 33 STT 194 Proper motion of B -018 -016. 08 48.4 +05 50 AGC 3 Rho Hya. A is a spectroscopic binary, P = 8.2d. 08 48.6 +02 37 A 2551 Too close 1933, 1944, 1954. Rapid motion. Quadrant ambiguity, but it appears that at least one revolution is complete. 08 48.7 +00 57 A 2552 P = 82yr., a = 0.24", motion retrograde. 08 48.9 +72 01 STF 1253 Proper motion of B +008 -009. 08 49.4 -62 16 HJ 4147 CD-61@2042. 08 49.5 +08 52 BU 1068 P = 195yr., a = 0.28", motion retrograde. 08 49.5 -20 54 J 1532 Hyderabad -21@ 8h 44m, Nos 43175-176. 08 49.8 +30 45 SEI 510 Proper motion of B -005 -015. 08 49.9 +14 50 STF 1283 Proper motion of B -018 +000. 08 50.0 +17 52 KU 33 Proper motion of B -058 -019. 08 50.3 -43 49 CPO 236 CPD-43@3034. 08 50.4 -00 02 HJ 3314 Proper motion of B -036 -065. 08 50.5 -38 13 JSP 307 A is variable. 08 50.7 +18 00 A 2473 P = 350yr., a = 0.425", motion direct. 08 50.7 +07 52 VDK 3 A premature orbit has been computed. 08 50.7 +04 01 STF 1286 Proper motion of B +016 -018. 08 50.8 +35 04 STF 1282 Proper motion of B -163 +099. 08 50.8 +34 18 AG 156 Proper motion of B +002 -020. 08 51.4 +20 53 STF 1285 Proper motion of B -028 -024. 08 51.6 -07 11 BU 587 15 Hya. A is a spectroscopic binary, and one component is variable. H 20 AC: H V 20. 08 52.0 +25 43 STT 96 B is BD+26@1854. Proper motion of B -045 -005. 08 52.1 -47 51 BRT 754 CPD-47@2847. 08 52.5 +28 16 HJ 460 53 Cnc. A is the variable BO Cnc. 08 52.6 +32 28 HU 1125 Sigma (1) Cnc. A spectroscopic binary. 08 52.6 +28 20 LDS 6219 55 Cnc. 08 52.6 -36 33 FIN 296 More than one revolution? 08 53.1 +54 57 A 1584 P = 71yr., a = 0.42", motion direct. 08 53.5 -46 03 CPO 241 CPD-45@3221. 08 53.8 -47 31 FIN 316 P = 7.2yr., a = 0.10", motion direct. Also a short- period spectroscopic binary. 08 53.9 -41 50 HJ 4150 Proper motion of B +007 -004. 08 54.0 +08 25 STT 195 57 Cnc. Proper motion of B -040 -002. 08 54.2 +30 35 STF 1291 Mt. Wilson spectral types G7,K0. 08 54.3 +12 39 HJ 109 Proper motion of B -004 +001. 08 54.6 +01 27 BAL 1430 Proper motion of B +000 -018. 08 54.9 +26 12 A 2131 P = 45yr. a = 0.34", motion direct. 08 55.2 -18 14 S 585 B is BD-17@2692. Proper motion of B -038 -002. 08 55.3 +46 56 HJ 1163 Proper motion of B -039 +008. 08 55.3 +32 47 AG 159 Proper motion of B +014 -018. 08 55.3 -11 22 S 584 B is BD-10@2691. Proper motion of B -002 +038. Optical. 08 55.5 -07 58 STF 1295 17 Hya. Both components are metallic-line stars. Proper motion of B +004 -040. 08 55.5 -27 41 SEE 107 Delta Pyx. 08 55.7 +41 41 A 2132 Round 1950-1968. Direct motion. 08 55.8 +64 58 ARG 21 A is an Algol-type system, AC UMa. Proper motion of B -002 -018. 08 55.9 +70 48 STF 1280 AB: Mt. Wilson spectral types M0, M0. Proper motion of A -1334 -362, B -1364 -407. AB: P = 680yr., a = 5.73", motion direct. 08 56.2 -55 32 DUN 73 B is CPD-55@1852. 08 56.3 -52 43 R 87 A is a spectroscopic binary. 08 56.7 +19 51 BLL 27 A is a semiregular variable, T Cnc. 08 57.0 -59 14 DUN 74 A variable, V376 Car. 08 57.4 -66 12 HJ 4164 Proper motion of B -035 +042 08 58.0 +30 14 HO 252 61 Cnc. Rapid binary? Measures scattered and uncertain. 08 58.5 +11 51 HJ 110 Alpha Cnc. A is an occultation double. 08 58.9 -47 14 HJ 4161 A is a Delta Scuti-type variable, FZ Vel. 08 59.2 +48 03 HJ 2477 Iota UMa. A is a Delta Scuti-type variable and spectroscopic binary. A-BC: A premature orbit has been computed. BC: P = 39.7yr., a = 0.68", motion retrograde. 08 59.5 +32 25 SHJ 100 Sigma (3) Cnc. B is BD+32@1820. 08 59.7 +03 31 BAL 2356 BAL 2356a. 08 59.8 +03 16 BAL 2356 BAL 2356b. 08 59.9 -01 35 HJ 111 Proper motion of B -062 +026. 09 00.1 -12 28 HU 225 P = 113yr., a = 0.30", motion direct. WOR 36 The faint companion may be physical. 09 00.3 +13 12 STF 1299 Proper motion of B -013 -002. 09 00.5 +32 25 HU 718 A premature orbit has been computed. 09 00.5 +06 17 RAB 1 Rabe identifies this as BDS 4887? Looks like another pair. 09 00.6 +41 47 KUI 37 P = 21.78yr., a = 0.647", motion retrograde. 09 00.8 +05 16 OSV 2 Ross 686,7. 09 01.3 +15 16 STF 1300 Proper motion of B -100 -334. 09 01.3 -38 55 I 1513 CPD-38@2898. 09 01.4 +32 15 STF 1298 66 Cnc. 09 01.8 +27 54 SHJ 101 67 Cnc. A is a spectroscopic binary. B is BD+28@1673. Proper motion of B -023 -029. 09 01.9 +26 12 STF 1301 Proper motion of B +018 +009. 09 03.2 -17 40 S 588 B is BD-17@2726. Proper motion of B +016 -008. 09 03.6 +47 09 A 1585 Both high and low eccentricity solutions have been computed: P = 36 or 74yr., a = 0.19 or 0.29", motion retrograde. 09 04.5 -57 40 RST 375 Spectral type G2? 09 05.1 +39 31 AG 160 Proper motion of B +018 -025. 09 05.6 +50 18 ES 2631 B is BD+50@1606. Proper motion of B +011 -018. 09 05.6 +01 03 BAL 1432 Proper motion of B -010 -002. 09 06.6 +02 49 STF 1309 Proper motion of B -038 +041. 09 07.1 +30 37 AG 162 BDS 4940, H N 30 may be same star. 09 07.4 +22 59 STF 1311 Proper motion of B -162 -016. 09 07.5 +11 36 J 1009 Proper motion of B -026 -043. 09 07.7 -44 38 I 492 A Beta Cephei-type variable. 09 07.8 -00 13 SCJ 12 Proper motion of B +002 -013. 09 07.9 -07 08 STF 1316 Proper motion of C +018 -017. 09 08.0 -25 52 I 491 Kappa Pyx. 09 08.0 -43 26 SEE 109 Lambda Vel. A is an irregular variable. 09 08.0 -64 02 HJ 4185 B is CPD-63@1097. 09 08.2 +23 53 POU 3029 Proper motion of B +001 -015. 09 08.4 +27 32 STT 97 B is BD+28@1698. Proper motion of B -045 +077. 09 08.6 -38 43 RST 1416 CPD-38@3012. 09 08.6 -48 41 LDS 251 B is CD-48@4456. 09 08.7 -08 35 KUI 38 19 Hya. A is a spectroscopic binary. 09 08.8 +26 38 STT 75 Cnc. A is a spectroscopic binary. B is BD+27@1716. 09 09.2 +15 14 STF 1317 Proper motion of B -006 -010. 09 09.4 +22 03 WRH 16 Xi Cnc. Uncertain binary, unresolved by speckle interferometry. A long-period spectroscopic binary. 09 09.6 -14 52 RST 3624 RST 3624a. 09 09.8 +11 34 CHR 131 Suspected occultation binary. 09 09.9 -30 22 H 96 H N 96. Epsilon Pyx. A is a spectroscopic binary. 09 10.0 -28 45 B 179 P = 77yr., a = 0.32", motion retrograde. 09 10.3 +52 23 STF 1312 Proper motion of B +002 000. 09 10.3 +22 00 WRH 17 79 Cnc. Less than 0.1" 1954 (Finsen); not resolved by speckle in 1983. Binary nature uncertain. 09 10.4 +67 08 STF 1306 Sigma (2) UMa. P = 1140yr., a = 6.39", motion retrograde. 09 10.4 +29 16 BOH 1 Proper motion of B +014 -007. 09 10.9 +63 31 H 73 H V 73. Tau UMa. A is a metallic-line star and long- period spectroscopic binary. 09 11.0 -19 29 I 824 Spectrum: Fm Delta Del. 09 11.1 +08 35 STF 1319 Proper motion of B -016 +004. 09 11.1 -60 57 FIN 129 Too close 1951,1954. 09 11.5 +28 01 HJ 805 Proper motion of B -046 -068. 09 11.9 +36 08 HJ 2483 Proper motion of B -007 +007. 09 11.9 +18 03 STT AB: 80 Cnc. BUP 124 BC: C is +18@2136. 09 12.3 +15 00 FIN 347 Aa: P = 2.70yr., a = 0.116", motion retrograde. A is Pi (1) Cnc. 09 12.4 +26 53 A 1977 1921-1922 elongation uncertain. Less than 0.1" in 1956. 09 12.4 -07 09 HJ 807 Proper motion of B -015 +014. 09 12.5 -43 37 FIN 317 Too close 1952-1968, with many negative observations by Finsen. 09 12.7 +61 56 STF 1314 The measure in BDS is evidently another pair; 1904.99, 126@.9, 36.26". 09 12.8 +61 41 STF 1315 B is BD+62@1055. Proper motion of B +005 +013. 09 12.8 -60 55 HDO 207 Aa-B: P = 71.3yr., a = 0.265", motion direct. 09 13.1 -41 28 CPO 41 A is CPD-40@3274, B is CPD-40@3273. 09 13.7 +11 09 HJ 122 Proper motion of B -008 -010. 09 14.2 -50 21 HJ 4192 B is CD-49@4232. Proper motion of B -014 +006. 09 14.3 -08 17 BU 908 B is BD-07@2762. 09 14.4 +52 41 STF 1321 Proper motion of A -1559 -570. B is BD+53@1321. Proper motion of B -1557 -656. A premature orbit has been computed. Both components are suspected spectroscopic binaries. 09 14.4 +02 19 HJ 2489 Theta Hya. Proper motion of B -033 +026. Optical. A is a spectroscopic binary. 09 14.9 +04 27 HEI 350 A long-period astrometric binary, now resolved. P = 29yr., a = 0.25", motion retrograde. 09 15.7 -01 14 STF 1329 An optical pair. B is BD-00@2163. Proper motion of B -025 -010. 09 15.8 -37 25 SEE 111 A is a spectroscopic binary. 09 16.1 -44 54 DON 329 Variable. 09 16.7 -06 21 KUI 40 23 Hya. A is a long-period spectroscopic binary. 09 16.7 -55 01 BRT 3291 CD-54@2689. 09 16.8 +23 55 POU 3039 Proper motion of B -100 +035. 09 16.8 +08 14 HJ 808 Proper motion of B +035 -075. 09 16.8 -21 57 I 493 Too close, position angle uncertain. 09 17.2 -22 49 J 1543 CD-22@7068. 09 17.3 -68 41 FIN 363 P = 3.20yr., a = 0.12", motion retrograde. 09 17.4 +23 39 STF 1332 Proper motion of B -052 -076. 09 17.5 +77 15 KUI 39 P = 71yr., a = 0.59", motion retrograde. Proper motion of A -1059 -020. 09 17.9 +28 34 STF 3121 P = 34.2yr., a = 0.66", motion direct. 09 17.9 +11 30 HJ 128 A is a spectroscopic binary. 09 17.9 -69 48 RMK 10 Proper motion of B +003 -012. 09 18.2 -00 36 HJ 126 Pettit measures for HJ 126: 1915.29, 132.6@, 93.9". It must be another pair. Proper motion of B -006 +008. 09 18.4 -20 22 S 595 B is BD-19@2673. Proper motion of B -043 -018. 09 18.6 +52 31 HJ 2492 AB: B is a faint nebula. 09 18.6 +20 49 HO 43 P = 155yr., a = 0.37", motion retrograde. 09 18.8 +36 48 STF 1334 38 Lyn. A is a spectroscopic binary. 09 19.3 +52 30 VBS 15 Identified as BDS 5000, HJ 2492 (Van Biesbroeck). May be another pair. 09 19.8 -11 58 B 2529 26 Hya. 1936, 1938 position angles 139@-122@. Distance 3.0". Invisible 1948 (van den Bos). 09 20.0 +05 00 STF 1343 Proper motion of B -069 -049. 09 20.5 -09 33 SHJ 105 27 Hya. A is a spectroscopic binary. Spectrum composite: G8III-IV+F5V. 09 20.7 +08 10 A 2976 Proper motion of B -042 +006. 09 20.7 -07 42 A 1082 P = 144yr., a = 0.51", motion retrograde. 09 21.0 +38 11 STF 1338 P = 390yr., a = 1.52", motion direct. 09 21.4 +81 23 STF 1304 B is BD+81@288. 09 21.5 -45 28 HJ 5452 HJ 5452a. 09 22.5 +49 33 STF 1340 Proper motion of B -031 -022. 09 22.6 +62 51 MLB 203 Proper motion of B -154 -052. 09 22.7 +50 36 STF 1341 Proper motion of B +055 +009. 09 22.8 -09 50 A 1342 P = 25.4yr., a = 0.28", motion direct. A magnetic and variable star, KU Hya, is in the system. 09 23.3 +03 30 STF 1347 Proper motion of B -062 +013. 09 23.6 -54 54 HJ 4207 B is CPD-54@2239. 09 23.8 +38 25 AG 164 Proper motion of B +026 +016. 09 24.5 +18 08 A 2477 P = 243yr., a = 0.35", circular orbit, motion direct. 09 24.7 +26 11 BU 105 Kappa Leo. 09 24.9 +51 34 STT 200 A is a spectroscopic binary. 09 25.3 -48 16 HJ 4209 B is CD-47@4921. 09 25.6 +54 01 STF 1346 Proper motion of B -019 -023. 09 25.7 -69 58 HJ 4216 B is CPD-69@1061. 09 26.0 +28 39 A 222 P = 127yr., a = 0.25", motion retrograde. 09 26.4 -29 27 COO 267 Proper motion of B -004 +050. 09 26.5 +78 26 STF 1326 Proper motion of B +023 +039. 09 26.5 -66 18 RST 404 CD-65@769. 09 27.1 -17 16 SKI 6 Proper motion of B -034 -052. 09 27.2 -09 13 A 1588 29 Hya. 09 27.6 -08 40 H 111 AB: H VI 111. Alpha Hya. B is BD-08@2681. 09 27.6 -35 00 B 2215 Last position angle uncertain. Needs speckle. 09 27.8 -06 04 B 2530 There may have been a quadrant reversal about 1951. P = 34.4yr., a = 0.38", motion direct. The 3 year spectroscopic motion does not seem to relate to the visual pair. 09 28.3 -78 15 HJ 4226 B is CPD-77@520. 09 28.5 +09 03 STF 1356 Omega Leo. P = 117yr., a = 0.88", motion direct. 09 28.5 +08 11 H 47 H IV 47. 3 Leo. Proper motion of B -015 -016. 09 28.5 -24 26 B 181 Not seen 1959-1962. May exhibit rapid retrograde motion. 09 28.7 +45 36 S 598 B is BD+46@1510. Proper motion of B +005 -032. 09 29.1 -02 46 HJ 1167 Tau (1) Hya. B is BD-02@2902. Proper motion of B +145 -025. 09 29.3 +03 06 BAL 2364 Proper motion of B -012 -018. 09 29.3 -44 32 DUN 77 B is CD-43@5332. Proper motion of B -095 +005. 09 29.7 +04 33 HJ 137 Proper motion of B -013 +007. 09 30.4 -58 22 RST 408 A is an irregular variable. 09 30.6 +10 36 STF 1360 Proper motion of B -188 -016. 09 30.7 +33 39 HJ 1166 7 LMi. Proper motion of B +027 -032. 09 30.7 -40 28 COP 1 Psi Velorum. P = 34yr., a = 0.80", motion direct. 09 30.8 -31 53 DUN 78 Zeta (1) Ant. 09 30.9 +73 26 HJ 2495 Proper motion of B -019 -011. 09 30.9 +44 41 STF 1358 B is BD+45@1729. Proper motion of B -034 -008. 09 31.2 +67 32 STF 1349 Proper motion of B +020 -020. 09 31.3 -13 29 KUI 41 Ross 440. P = 18.3yr., a = 0.55", motion retrograde. The primary is probably a flare star. 09 31.7 +38 30 AG 168 BD+39@2255a. 09 31.5 +63 04 STF 1351 23 Uma. Proper motion of B +088 +023. The primary is a Delta Scuti-type variable. 09 32.0 +20 03 STF 1364 Proper motion of B -042 -023. 09 32.0 +09 43 SHJ 107 6 Leo. A is a spectroscopic binary. B is BD+10@2015. Proper motion of B -012 -017. 09 32.0 -01 11 CHR 174 Tau (2) Hya. A spectroscopic binary, now probably resolved. 09 32.2 -62 47 FIN 140 A is a Mira-type variable, R Car. 09 32.7 +01 52 FIN 349 P = 37yr., a = 0.29", motion direct. 09 32.7 -28 26 I 1616 B is CD-27@6693. B is variable. 09 32.8 -57 06 SYO 1 Spectral type B6/7II/III. 09 32.9 +51 41 BU 1071 Theta UMa. A is a spectroscopic binary. 09 33.1 -39 08 JC 21 B is CD-38@5675. Proper motion of B -026 +041. 09 33.3 +28 22 H 29 H N 29. 09 33.3 -86 01 DUN 82 Proper motion of B -048 -020. 09 33.6 -49 45 DUN 79 B is CD-49@4504. Proper motion of B +062 -003. 09 34.1 +38 26 HJ 2499 ALI 845. Schembor measures 1926.28, 290.4@, 31.73". 1900: 09 28.2 +38 51. 09 34.3 +66 48 STF 1350 Proper motion of B -008 -026. 09 34.7 -12 36 STF 1370 B is BD-11@2669. Proper motion of B -028 +005. 09 35.0 -43 39 DON 344 CPD-43@3821. 09 35.2 +14 05 STT 102 B is BD+14@2114. Proper motion of B -025 -058. 09 35.3 -10 19 LDS 6229 B is BD-09@2878. 09 35.4 +39 58 COU 2084 A is a spectroscopic binary. 09 35.4 +03 54 STF 1371 Proper motion of B -054 -072. 09 35.6 -19 35 S 604 B is BD-18@2729. 09 35.7 +53 18 STF 1366 Proper motion of B -031 -033. 09 35.7 +35 49 HU 1128 11 LMi. Companion not seen 1941-1958 (Van Biesbroesk 82-inch). P = 201yr., a = 3.84", motion retrograde. Proper motion of B -724 -239. A is slightly variable, SV LMi, P = 18d, probably due to starspots. 09 35.9 +14 23 H 58 H V 58. 7 Leo. Proper motion of B -047 -008. B is BD+15@2078. 09 36.0 -27 31 B 185 Proper motion of B -039 -001. 09 36.1 +53 18 STF 1368 Proper motion of B -006 +003. 09 36.4 -48 45 R 125 A is the variable IM Vel. 09 36.7 -41 45 BRT 765 CPD-41@3877. 09 36.8 +19 14 HJ 468 Proper motion of B -035 -023. 09 37.6 +15 28 A 2479 P = 108yr., a = 0.23", motion direct. 09 37.8 -40 31 CPO 267 CPD-39@3770. 09 37.9 +45 54 A 1765 Round or single 1934-1951, 1966-1968. Possibly am- biguous case: P = 28.2 or 52.7yr., a = 0.15 or 0.19", motion retrograde. 09 39.4 -57 31 RST 419 Spectral type G8/K0II/III. 09 40.4 +19 36 KU 98 Proper motion of B -022 +005. 09 40.7 -57 59 B 780 P = 10.7yr., a = 0.14", motion retrograde. 09 40.9 -49 13 R 128 B is CD-48@4895. 09 41.2 +09 54 WGT Omicron Leo. H 76 H VI 76. 09 41.3 -23 35 H 20 H N 20. 09 41.6 +15 32 LDS 3915 The primary is the variable DR Leo. 09 42.2 -66 55 HJ 4241 B is CPD-66@1039. 09 42.5 +18 13 HJ 2502 Proper motion of B +001 -007. 09 43.1 -81 20 R 133 B is CPD-80@388. 09 43.2 +67 09 MLR 323 Proper motion of B -057 +007. 09 43.5 -51 14 B 1658 A is the variable IP Vel. 09 43.7 +14 01 BUP 128 Psi Leo. 09 43.8 +55 57 ES 1825 A is W UMa, prototype of its class. A distant star, BD+55@1351, may have common proper motion and radial velocity. 09 44.2 -27 46 FIN 326 Theta Ant. P = 18.3yr., a = 0.13", motion retrograde. Spectrum composite; A8V+F7II-III. 09 44.5 +48 30 HJ 2503 B is BD+49@1874. 09 45.0 -49 29 DUN 80 B is CD-48@4963. Proper motion of B -017 +084. 09 45.1 -45 03 CPO 271 Proper motion of B -082 +038. 09 45.9 +63 39 KUI 43 28 UMa. A is a spectroscopic binary. 09 46.1 -23 01 DON 1086 CD-22@7568. 09 47.1 -65 04 RMK 11 Upsilon Car. 09 47.4 +11 34 MCA 34 19 Leo. P = 15.7yr., a = 0.112", motion direct. 09 47.7 -37 36 JSP 348 CPD-37@3758. 09 47.8 -65 07 HJ 4252 B is CPD-64@1087. 09 49.5 -10 33 A 1344 P = 126yr., a = 0.33", motion retrograde. 09 49.8 +21 11 KUI 44 20 Leo. B is a Delta Scuti-type variable, DG Leo. A is a spectroscopic binary. 09 49.9 +16 20 STF 1384 Proper motion of B -004 -035. 09 50.0 -45 44 HJ 4254 B is CD-45@5471. 09 50.4 -50 11 HJ 4257 B is CD-49@4737. 09 50.8 +11 51 J 389 21 Leo. 09 50.8 +03 41 A 3081 Less than 0.1" in 1956. Not seen double since 1935. 09 51.0 +59 02 STT 521 Upsilon UMa. A is a Delta Scuti-type variable. 09 51.2 +36 29 HO 369 P = 117yr., a = 0.19", motion direct. 09 51.9 -60 26 HJ 4263 Proper motion of B +003 -040. 09 52.1 +54 04 STT 208 Phi UMa. P = 105.4yr., a = 0.35", motion direct. 09 52.2 +03 13 BAL 2368 Proper motion of B -022 +009. 09 52.5 -08 06 AC 5 Gamma Sex. P = 77.6yr., a = 0.38", motion retrograde. 09 53.0 -77 48 RST 1468 Spectrum: A3/4II/III. 09 53.1 -55 01 R 137 B is CPD-54@2822. 09 54.1 +04 57 S 605 9 Sex. B is BD+05@2247. Proper motion of B -040 -012. 09 54.3 -45 17 DUN 81 Proper motion of B -015 +003. 09 54.8 -52 05 HJ 4266 Proper motion of B -009 000. 09 55.1 +68 54 STF 1387 Proper motion of D -058 -061. 09 55.4 +10 07 STF 1395 Proper motion of B -067 -001. 09 56.9 -54 34 I 396 Psi Vel. 09 57.0 +19 46 STF 1399 B is BD+20@2400. Proper motion of B -236 -002. 09 57.3 -29 02 WHC 30 B is CD-28@7774. Proper motion of B +066 -051. 09 57.7 -48 25 HJ 4269 A is a spectroscopic binary. 09 57.9 -60 45 FIN 152 Spectrum of B is A/F. 09 58.4 -01 35 HJ 147 Proper motion of B +019 -002. 09 58.7 +10 58 H 63 H V 63. 09 58.9 -35 53 HJ 4271 Eta Ant. 09 59.1 +53 16 A 1346 P = 129yr., a = 0.28", motion retrograde. 09 59.1 -23 26 BRT 1481 CD-22@7789. 09 59.4 -23 29 BRT 1482 CD-22@7794. 09 59.4 -44 57 HJ 4273 Equal double lines in the spectrum of A. 09 59.8 -21 28 DON 376 CPD-20@4801. 09 59.8 -59 16 HJ 4278 B is CPD-58@1765. 10 00.0 +24 33 CHR 145 The CHARA companion is apparently the third component in the system, as reported previously (Astron. J. 89, 683). The primary is DH Leo, a RS CVn system, and spectroscopic binary with a period of 1.07d. 10 00.2 +06 15 STF 1401 Proper motion of B -129 +010. 10 01.1 -41 54 CPO 279 CPD-41@4230. 10 01.2 -56 06 HDO 209 B is CPD-55@2795. 10 01.9 +73 34 STF 1393 Proper motion of B +004 -007. 10 01.9 -28 41 HJ 4277 B is CD-28@7839. Proper motion of B -054 +035. 10 02.1 -54 59 DUN 83 B is CPD-54@3041. Proper motion of B -015 +003. 10 02.3 -43 38 I 1522 Too close 1930-1936 and not observed since. 10 02.9 +68 47 STF 1400 Very similar in characteristics to STF 1398. Observers have confused them. 10 03.2 -52 03 HJ 4282 B is CD-51@4435. Proper motion of B -023 -017. 10 03.4 +57 32 A 1347 The scattered measures show evidence of rapid motion. 10 04.1 +16 27 BRT 1266 Proper motion of B -003 -002. 10 04.1 -76 04 HJ 4288 B IS CPD-75@634. Proper motion of B -049 +006. 10 04.3 -01 42 STF 1404 Proper motion of B -059 -016. 10 04.3 -28 23 I 292 A premature orbit has been computed. 10 04.9 +55 29 STF 1402 Proper motion of B +076 -015. 10 06.1 +03 03 BAL 2369 Proper motion of B +003 -011. 10 06.2 -41 45 RST 1478 Proper motion of B +017 -023. 10 06.2 -47 22 I 173 P = 232yr., a = 0.64", motion direct. 10 06.5 +43 33 WEI 22 Proper motion of B -001 -003. 10 06.6 -19 19 S 607 Proper motion of B +037 -021. 10 06.7 -70 45 NZO 15 Nothing at this position (Heintz). The spectral type of -70@964 is K1/2III/IV. 10 06.8 +05 37 CHR 30 14 Sex. 10 07.2 -22 20 RST 3679 CPD-21@4616. 10 07.3 +16 46 WRH 18 Eta Leo. Occultation binary now confirmed by speckle. 10 07.5 -59 04 COO 97 B is CPD-58@1922. Proper motion of B -021 +004. 10 07.9 +10 00 GAN 5 31 Leo. 10 08.3 +31 36 KUI 48 P = 17.76yr., a = 0.156", motion direct. 10 08.4 +11 58 STF 6 Alpha Leo. 10 08.5 +68 26 ENG 41 B is BD+69@557. 10 08.7 -65 49 HJ 4292 B IS CPD-65@1250. 10 09.0 +64 27 STF 1407 Proper motion of B -021 -027. 10 09.3 +20 20 A 2145 P = 71yr., a = 0.13", motion retrograde. 10 10.0 +16 23 A 2367 Proper motion of B -128 -008. 10 10.6 -12 21 BU 593 Lambda Hya. A is a spectroscopic binary. 10 11.0 +75 08 KUI 47 P = 175yr., a = 1.58", motion direct. 10 11.0 -48 14 BRT 775 CPD-47@3979. 10 11.2 +76 22 HJ 3319 Proper motion of B -056 -048. 10 11.4 +73 02 STF 1408 Proper motion of B +008 +026. 10 11.4 +49 27 ENG 42 AB: Proper motion of A -1353 -501. Slightly variable. BUP 130 BC: C is BD+50@1723. Proper motion of C +001 -024. 10 11.6 +13 21 HU 874 Too close to measure 1949-1956. P = 20.5yr., a = 0.155", inclination 90 degrees. 10 12.0 -06 12 HO 44 Motion in a highly-inclined orbit. 10 12.1 +21 18 A 2146 P = 98yr., a = 0.22", motion direct. 10 12.3 -16 05 STF 1416 Proper motion of B +014 +007. 10 13.1 +27 25 STT 213 P = 158yr., a = 0.84", motion retrograde. 10 13.4 -50 54 HJ 4299 B is CD-50@4922. 10 14.5 -68 52 GLI 133 Proper motion of B -002 +008. 10 15.1 -67 17 CPO 48 C is probably CPD-66@1208. 10 15.2 +01 34 BAL 1872 BD +02 2309a. 10 16.1 -59 54 HU 1597 P = 92yr., a = 0.39", motion direct. 10 16.3 +17 44 STT 215 P = 670yr., a = 1.34", motion retrograde. 10 16.3 -28 59 I 851 P = 90yr., a = 0.30", motion retrograde. 10 16.7 +57 37 HJ 1176 Proper motion of B -056 -030. 10 16.7 +23 25 STF 18 Zeta Leo. A spectroscopic binary. B is BD+29@2207. Proper motion of B -209 +039. 10 16.9 +25 52 BUP 131 B is BD+26@2062. Proper motion of B -089 -007. 10 17.1 -61 20 B 1673 Variable, V337 Car. 10 17.2 +23 06 STT 523 39 Leo. Mt. Wilson spectral types are F1s and dM1. 10 17.8 +71 04 STF 1415 Proper motion of B -030 -042. 10 18.0 -02 42 BAL 208 Proper motion of B -022 -001. 10 18.3 -03 26 RST 4454 Round 1958 with 82-inch. 10 18.9 +44 03 ENG 43 B is BD+44@1975. Proper motion of B +029 -052. 10 19.2 +20 34 STF 1423 P = 460yr., a = 1.48", motion retrograde. 10 19.6 +19 52 BAG Resolved in the infrared by speckle interferometry. This is the flare star AD Leo, which has been reported to be an astrometric binary (uncertain). 10 19.6 -57 24 FIN 162 A is the Algol-type system HP Car. 10 19.8 -30 36 RST 2685 Corrected position and Durchmusterung number (Heintz). 10 20.0 +19 50 STF 1424 Gamma Leo. AB: Premature orbits have been computed. C is an optical companion, and is the flare star AD Leo. Speckle by Balega et al showed no companion 1987.3827. D is BD+20@2464. 10 20.4 +68 08 HJ 3324 Proper motion of B -025 -019. 10 20.6 -23 38 HJ 4305 Proper motion of B -038 -030. 10 20.8 +58 36 A 1349 Proper motion of B +004 +001. 10 20.8 -67 32 HJ 4314 B is CPD-66@1232, spectrum B9/A0IV/V. Proper motion of B -017 000. 10 20.9 -56 03 RMK 13 A has a variable spectrum. 10 21.8 -44 30 LDS 6232 B is CD-43@6191. 10 22.0 +43 54 STF 1427 Proper motion of B -045 -005. 10 22.4 -47 58 HJ 4312 Proper motion of B +005 000. 10 22.7 +15 21 STT 216 P = 306yr., a = 1.74", motion retrograde. 10 23.2 +05 42 SHJ 115 Proper motion of B +006 -009. 10 23.6 -29 34 HJ 4313 Proper motion of B +048 +026. 10 23.6 -44 08 HJ 4315 B is CD-43@6220. 10 23.7 +02 37 LAM B is BD+03@2357. Proper motion of B -031 +025. 10 24.4 +34 11 STT 104 B is BD+34@2122. Proper motion of B -003 -017. The primary is a semi-regular variable. 10 25.0 +24 37 STF 1429 A premature orbit has been computed. 10 25.7 -07 04 SCA 53 Spectrum: K5:IIIbFe-0.5. 10 26.0 +52 37 STF 1428 BDS 5386, H I 71 probably same star. 10 26.2 +03 56 BU 1280 A is a Delta Scuti-type variable, RX Sex. 10 26.3 -53 53 HJ 4319 Spectrum M2IabCN0.5, variable in light. 10 26.3 -55 29 R 146 Proper motion of B -013 -022. 10 26.9 +19 31 COU 292 P = 21.7yr., a = 0.16", motion retrograde. 10 26.9 +17 13 STT 217 P = 140yr., a = 0.42", motion direct. 10 27.1 +18 04 STF 1434 Proper motion of B -113 -103. 10 27.2 -47 25 CPO 291 Proper motion of B +014 -006. 10 27.6 +09 46 HJ 832 45 Leo. A is an Alpha CVn-type variable, CX Leo, and a spectroscopic binary. 10 27.9 +36 42 HU 879 Beta LMi. P = 37.9yr., a = 0.34", motion direct in a highly-inclined orbit. 10 28.0 +19 50 STF 1435 Proper motion of B -072 -010. 10 28.2 -25 48 FIN 308 P = 67yr., a = 0.17", motion direct. C is physical. 10 28.4 +03 10 CHE 148 Proper motion of B +007 +002. 10 28.8 -62 35 DUN 85 B is CPD-61@1676. Proper motion of B -008 +002. 10 29.1 +03 42 BAL 2841 Proper motion of B -055 -018. 10 29.6 -30 36 H 50 H N 50. Delta Ant. 10 29.9 +28 35 STT 105 B is BD+29@2056. 10 30.2 +51 00 STT 219 BDS 5471, HJ 2535 probably same star. 10 30.6 +55 59 LDS 2863 B is BD+56@1458. 10 30.7 -54 29 HJ 4327 B is CPD-53@3900. Proper motion of B +001 +003. 10 30.7 -61 21 DUN 87 B is CPD-60@1944. Proper motion of B -012 +002. 10 31.0 -07 38 STF 1441 A is a spectroscopic binary. C is BD-06@3171. 10 31.3 -51 53 HJ 4328 B is CD-51@4816. 10 31.4 -53 43 HJ 4329 Proper motion of B +003 -009. 10 31.6 -39 56 HJ 4326 B is CD-39@6453. 10 31.7 +02 35 HJ 2533 Proper motion of B +004 -032. 10 31.7 -44 29 B 1161 Measures uncertain, too close. Needs speckle. 10 31.9 +32 23 HJ 482 33 LMi. 10 31.9 -81 55 HJ 5444 B is CPD-81@448. Proper motion of B -017 -004. 10 32.0 +22 02 STF 1442 Proper motion of B -005 +006. 10 32.0 -45 04 PZ 3 B is CD-44@6582. Proper motion of B -006 -034. 10 32.6 +80 55 HU 878 Proper motion of B +038 -015. 10 32.8 +09 18 WRH 19 Rho Leo. Possible spectroscopic binary. 10 32.9 -47 00 HOR 1 Aa-B: B is CD-46@6207. 10 33.2 +40 26 HJ 2534 A is a spectroscopic binary. 10 33.5 -46 59 HJ 4332 B is CD-46@6218. 10 33.6 +15 13 STF 1446 Proper motion of B +006 -002. 10 33.8 +23 21 STF 1447 Proper motion of B -041 +010. 10 33.9 -17 50 S 610 B is BD-17@3179. 10 34.0 -23 45 BU 1269 44 Hya. 10 34.5 -17 53 B 2533 Perhaps identical with HLD 107. 10 35.0 +08 39 STF 1450 49 Leo. A is the Algol-type system TX Leo. 10 35.1 -57 41 COO 107 Spectrum of B is A. 10 36.1 +11 37 BIG 1 B is BD+12@2234. Proper motion of B -089 +007. 10 36.1 -26 41 BU 411 P = 210yr., a = 0.98", motion retrograde. 10 36.3 -16 21 BU 1075 Phi (2) Hya. 10 36.8 -13 32 STF 1453 Proper motion of B -008 +047. 10 37.0 -08 50 A 556 A premature orbit has been computed. 10 37.3 -48 14 SEE 119 P = 16.5yr., a = 0.38", motion retrograde. A is a spectroscopic binary. 10 37.5 -09 32 RST 3708 P = 78.5yr., a = 0.22", motion direct. 10 37.6 -45 56 CPO 296 CPD-45@4802. 10 37.7 -73 35 HJ 4344 B is CPD-72@998. 10 38.3 +60 07 STT 222 A is a spectroscopic binary. 10 38.3 +01 15 STF 1456 Proper motion of B -007 -017. 10 38.6 -45 58 B 2715 CPD-45@4816. 10 38.7 -59 11 DUN 94 Proper motion of B -012 -013. 10 39.0 -58 49 GLI 152 B is CPD-58@2475. Proper motion of B -015 +004. 10 39.5 +31 42 STF 1458 Proper motion of B -099 -038. 10 39.7 +08 51 STT 224 P = 235yr., a = 0.56", motion retrograde. 10 40.2 -16 22 LDS 311 B is BD-15@3101. Proper motion of B +101 -080. 10 40.6 -59 33 COO 110 B is CPD-58@2523. 10 40.9 -35 45 B 2001 Spectrum composite; G8-K0III+F-G. 10 41.6 -00 16 STF 1464 Proper motion of B -013 -028. 10 42.2 +31 42 BLL 28 A is the semiregular variable RX LMi. 10 42.2 +23 34 POU 3086 Proper motion of B -008 +007. 10 42.6 +03 35 A 2768 P = 80.6yr., a = 0.378", motion retrograde. 10 42.9 +50 48 STF 1462 Proper motion of B -009 +002. 10 42.9 -00 06 BAL 1155 Proper motion of B -037 -022. 10 43.0 +26 20 BU 913 40 LMi. 10 43.2 -61 10 DUN 97 Proper motion of B -022 +016. 10 43.3 +04 45 STF 1466 35 Sex. Proper motion of B +030 -024. A is a spectroscopic binary. Spectrum composite; K3III+K0III. 10 43.5 +46 12 SMA 75 B is BD+46@1658. Proper motion of B -265 -064. B is a spectroscopic binary. 10 43.8 -59 57 HJ 4355 B is CPD-59@2547. 10 44.1 -59 35 HJ 4360 Proper motion of C +004 000. 10 44.3 -45 15 CPO 301 B is CD-44@6765. 10 44.3 -70 52 DUN 99 B is CPD-70@1185, spectrum A6IV. 10 44.4 -60 00 DAW 8 Often classified O9 or 9.5. QZ Car. The bright star consists of two eclipsing pairs, P = 20.73d and 6.00d. 10 44.6 -59 44 BSO 4 A is a spectroscopic binary. B is CPD-59@2584. 10 44.7 -60 01 HJ 4363 B is CPD-59@2593. 10 45.1 -59 41 B 2256 Eta Car, an old nova in a nebula with nuclei. Variable. 10 45.3 -59 45 COO 113 B is CPD-59@2633. 10 45.3 -80 28 I 294 Delta (1) Cha. 10 45.4 -43 42 HJ 4362 B is CD-43@6533. 10 45.7 -01 30 FIL 26 Proper motion of B -011 -035. 10 45.8 -59 29 HJ 4369 B is CPD-58@2685. A is an irregular variable, BO Car. 10 45.9 +30 41 S 612 42 LMi. B is BD+31@2181. Proper motion of B -038 -042. 10 46.1 -56 57 HRG 133 B is CPD-56@3776. 10 46.1 -59 34 HJ 4370 B is CPD-58@2689. 10 46.3 -60 36 RST 4463 A is a spectroscopic binary. 10 46.6 -59 33 HJ 4371 B is CPD-58@2700. 10 46.8 -49 25 R 155 Mu Vel. P = 138yr., a = 1.43", motion direct. A is a spectroscopic binary. 10 46.9 -41 56 COO 114 Proper motion of B -016 -006. 10 47.0 +13 02 STF 1472 Proper motion of B +007 -014. 10 47.2 -60 06 COO 115 B is CPD-59@2700. 10 47.6 -15 38 STF 1473 B is BD-14@3187. Proper motion of B -116 -047. 10 47.7 +65 28 STF 1469 Proper motion of B -104 -007. 10 48.1 +13 13 AG 341 Proper motion of B -007 -006. 10 48.5 -22 23 RST 2710 CPD-21@4800. 10 49.3 -04 01 STF 1476 40 Sex. 10 49.3 -46 52 BRT 790 CPD-46@4866. 10 49.3 -68 45 HJ 4351 Proper motion of B -255 -195. 10 49.6 +12 56 STF 1477 Proper motion of B -039 -062. 10 49.6 -35 52 JC 22 B is CD-35@6767. 10 50.3 -08 54 HJ 838 41 Sex. A is a spectroscopic binary. C is BD-08@3019. 10 50.6 -41 12 CPO 306 Nys calls A CPD-40@4776, and B CPD-40@4775. 10 51.0 -59 57 HJ 4378 B is CPD-59@2783. 10 51.6 +06 35 J 80 Proper motion of B -037 -011. 10 51.6 -21 15 BU 1428 A is the variable V Hya. Proper motion of B -003 +004. 10 52.0 +16 06 A 2373 P = 93yr., a = 0.15", motion retrograde. 10 52.0 +09 04 A 2772 Proper motion of B +021 -042. 10 52.2 +07 28 STF 1482 Proper motion of B +005 -043. 10 53.4 +13 26 HJ 2547 Proper motion of B -016 +013. 10 53.4 -02 15 S 617 BDS 5610 is probably identical (BDS). B is BD-01@2458. A is a spectroscopic binary. Proper motion of B -136 -083. 10 53.5 -20 08 BU 1429 A is a long-period variable, V Hya. 10 53.5 -58 51 DUN 102 B is CPD-58@2830. Proper motion of B -013 +002. 10 54.6 -38 45 HJ 4381 B is CD-38@6819. Proper motion of B -016 000. 10 55.0 +52 07 STF 1486 Proper motion of B +004 +016. 10 55.6 +24 45 STF 1487 54 Leo. B is a spectroscopic binary. 10 55.7 +00 44 BU 1076 55 Leo. P = 128yr., a = 0.82", motion retrograde. 10 55.7 -46 25 CPO 309 CPD-45@5026. 10 56.1 -21 08 S 618 B is BD-20@3300. 10 56.2 +48 02 ES 2636 B is BD+48@1901. One component is variable. 10 56.4 -57 33 HJ 4387 B is CPD-56@4017. 10 57.0 -00 51 LDS 6235 Proper motion of B +064 -140. 10 57.0 -71 21 HJ 4392 B is CPD-70@1261. 10 58.2 -31 34 HJ 4389 Proper motion of B -040 -009. 10 58.3 +13 17 STF 1496 Proper motion of B -018 -016. 10 58.5 +17 11 A 2375 P = 150yr., a = 0.38", motion retrograde. 10 58.6 +09 08 STF 1497 Proper motion of B -025 -006. 10 59.4 -43 08 HJ 4394 B is CD-42@6636. 10 59.8 +58 54 STF 1495 B is BD+59@1339. Proper motion of B -019 -003. 11 00.6 +38 32 ES 304 ALI 1090 is not present (Heintz). 11 00.6 +03 37 CHR 33 58 Leo. Also an occultation binary. 11 00.6 -18 19 HJ 1181 A is the semiregular variable R Crt. B is BD-17@3279. 11 00.7 +06 06 BU 598 59 Leo. 11 01.2 +21 05 WEI 26 Proper motion of B -049 +001. 11 02.0 +14 37 STF 1502 Proper motion of B -068 +025. 11 02.1 -15 42 H 177 H I 177. 11 02.2 +09 54 STF 1503 A is the W UMa-type system AM Leo. Proper motion of B -030 -042. 11 02.2 +09 45 HJ 172 Proper motion of B -078 +021. 11 02.4 -26 50 B 208 Too close, with few measures. Needs speckle. 11 02.8 -59 44 JSP 455 The primary is variable. 11 03.5 +54 32 A 1590 P = 202yr., a = 0.86", motion retrograde. 11 03.7 +61 45 BU 1077 Alpha UMa. P = 44.4yr., a = 0.60", motion retrograde. Faint, distant pair (BU) 1881.12, 203.5@, 384.9", 7.60V. Possible common proper motion with the spectroscopic binary HD 95638 at 280". 11 03.7 +32 53 HJ 493 Position by Espin is 1 minute greater in right ascen- sion than John Herschel's. Used Espin position. 11 04.5 +38 14 HO 377 51 UMa. 11 04.7 -04 13 STF 1506 A-BC: A is physical. A 676 BC: P = 23.6yr., a = 0.28", motion direct. 11 05.0 +07 20 KUI 54 Chi Leo. 11 05.1 -59 43 GLI 159 Proper motion of B +001 +001. 11 05.3 -27 18 FIN 47 Chi (1) Hya. P = 7.40yr., a = 0.14", motion retrograde in a highly-inclined orbit. 11 05.5 +43 32 VBS 18 Proper motion -4405 +940. The companion is WX UMa. 11 05.6 +54 48 A 1591 P = 105yr., a = 0.20", motion retrograde. 11 05.7 +62 37 STF 1505 Proper motion of B +006 -011. 11 06.1 +13 25 BRT 1271 Declination corrected by Heintz. 11 06.1 +07 02 STF 1507 Proper motion of B -010 -051. 11 06.5 -13 25 STF 1509 B is BD-12@3347. Proper motion of B -003 -023. 11 06.5 -58 41 HDO 210 A is variable. 11 06.9 +01 57 BU 599 65 Leo. 11 07.2 +57 11 HJ 2556 Position correction by Heintz. 11 07.2 +10 55 STF 1511 Proper motion of B +043 +036. 11 07.3 +28 32 HJ 1185 C is a faint nebula (HJ 820). Distance 259.4". 11 07.3 -42 38 HJ 4409 The variable V815 Cen. 11 07.4 -48 15 CPO 316 B is CD-47@6520. 11 07.6 +43 29 HJ 2557 Proper motion of B +004 -006. 11 08.0 +52 49 STF 1510 Proper motion of B -043 -004. 11 08.4 +03 13 H 68 H V 68. B is BD+03@2462. 11 08.8 +24 40 A 677 67 Leo. 11 09.2 +62 30 STF 1512 Proper motion of B +004 -054. 11 09.2 -18 51 B 2007 Not seen in 1938 (Finsen). 11 09.5 +83 06 STF 1499 Proper motion of B -063 -036. 11 09.8 +63 20 H 106 H IV 106. 11 10.3 +38 40 HJ 2561 A measure by Schembor: 1926.08, 172.6@, 23.24". 11 10.6 +64 44 HZG B is BD+65@820. 11 10.7 +31 10 HJ 2562 A premature orbit has been calculated. 11 10.8 +64 43 MLB 408 Proper motion of B -035 -010. 11 11.1 +30 27 STT 231 Mt. Wilson spectral types M1, M2, G5. 11 11.4 -09 21 STF 3068 Proper motion of B -012 -001. 11 12.1 -71 26 B 2273 A may be variable. 11 12.5 +35 49 STT 108 BD: Distances 2083.6" and 2094.6". D is BD+36@2170. Proper motion of D +012 +010. 11 12.5 -18 30 BU 220 Psi Crt. P = 186yr., a = 0.47", motion retrograde in a highly-inclined orbit. 11 12.5 -49 05 CPO 319 CPD-48@3801. 11 13.1 +40 11 HJ 494 Proper motion of B -022 -016. 11 13.3 +38 11 KU 36 Proper motion of B +012 +003. 11 13.5 -55 26 HJ 4417 B is CPD-54@4398. 11 13.6 +55 25 A 1353 P = 124yr., a = 0.38", motion retrograde. 11 13.6 -15 58 ARG 24 Proper motion of B -016 +000. 11 13.7 +20 08 STF 1517 Alternate spectral types G5III, G7IV. Slightly variable. 11 14.1 +20 31 STT Delta Leo. Variable? 11 15.0 -54 20 BRT 2062 CD-53@3941. 11 15.1 -39 29 SEE 128 Direct motion. 11 15.2 +73 29 STF 1516 Proper motion of B -002 -007. STT 539 Proper motion of C -362 +067. 11 15.4 -18 07 LDS 342 B is BD-17@3337. Proper motion of B +132 -726. 11 15.7 +45 51 STT 109 B is BD+46@1707. Proper motion of B -010 -023. 11 15.7 -16 21 SHJ 372 B is BD-15@3226. Proper motion of B -001 +004. 11 15.9 +13 18 MCA 35 73 Leo. A spectroscopic binary now resolved by speckle interferometry. 11 16.1 +52 46 STF 1520 Proper motion of B +172 +060. 11 16.5 +26 27 BUP 137 B is BD+27@2000. Proper motion of B -032 -016. 11 16.6 -52 15 RST 2737 RST 2737a. 11 16.7 -03 39 SHJ 121 Phi Leo. B is BD-02@3314. Proper motion of B +004 -051. 11 17.0 -07 08 BU 600 A is an Alpha CVn-type variable, SV Crt., and a spectro- scopic binary. 11 17.3 -67 49 DON 471 A is variable. 11 17.5 -59 06 R 163 Spectrum B9.5/A0III. 11 17.9 -40 34 I 1538 Measures uncertain. 11 18.2 +31 32 STF 1523 Xi UMa. P = 59.8yr., a = 2.53", motion retrograde. A is known to have an unseen companion, P = 1.83yr. B is a spectroscopic binary. 11 18.5 +33 06 STF 1524 Nu UMa. 11 18.5 +00 25 BAL 1158 Proper motion of B -036 +027. 11 18.7 +02 50 STF 1526 B is BD+03@2482. Proper motion of B -085 -064. 11 19.0 +51 18 WNC 3 Proper motion of B +045 -006. 11 19.0 +14 16 STF 1527 A premature orbit has been computed. 11 19.1 +38 11 CHR 133 55 UMA. A short-period spectroscopic binary, P = 2.5d. The speckle pair must be different, hence a triple. 11 19.4 -01 39 STF 1529 Proper motion of B -186 -148. 11 19.4 -64 35 LDS 6242 A is CD-63@643. 11 19.7 -06 54 STF 1530 Proper motion of B -123 +041. 11 20.6 -27 18 BRT 2986 CPD-26@4502. 11 21.0 -54 29 I 879 Pi Cen. P = 39.2yr., a = 0.28", motion direct. 11 21.1 -35 31 I 1539 Position angle uncertain. Needs speckle. 11 22.1 +37 05 STF 1533 B is BD+37@2177. Proper motion of B +025 -026. 11 22.1 -24 47 I 507 Direct motion. 11 22.6 -51 34 LDS 351 B is CD-50@5949. 11 22.9 +00 56 STF 1535 Proper motion of B -036 +010. 11 23.0 +04 08 A 2776 P = 68yr, a = 0.24", motion direct. C is physical. 11 23.1 -10 20 OL 12 Not found in 1939. Position may be in error (van den Bos). 11 23.7 -28 31 ARG 25 B is CD-27@8061. 11 23.9 +10 32 STF 1536 Iota Leo. P = 183yr., a = 1.93", motion retrograde. Mt. Wilson spectral types F3s and F3s. A is a Delta Scuti-type variable. 11 23.9 -23 19 RST 2746 CD-22@8867. 11 24.4 +06 20 HJ 2569 Position correction by Heintz. 11 24.5 -04 23 STF 3070 Proper motion of B -081 -045. 11 24.7 -61 39 BSO 5 P = 421yr., a = 5.76", motion direct. 11 24.9 -17 41 HJ 840 Gamma Crt. 11 25.0 -52 36 RST 541 RST 541a. 11 25.2 +16 08 HEI 156 There is a third star at 46@, 25". 11 25.6 +16 27 HJ 4433 81 Leo. 11 26.2 -22 41 B 1697 Proper motion of B -044 +011. 11 26.8 +59 23 FOX 171 Position of ADS 8161, referred to BD+60@1328. 11 26.8 +03 01 STF 1540 83 Leo. B is BD+03@2503. Proper motion of B -727 +189. 11 26.8 -53 10 I 883 Spectrum composite; K0III+A2-3V. 11 27.0 -54 51 HJ 4436 B is CPD-54@4542. 11 27.2 +19 08 KU 38 Proper motion of B -038 -017. 11 27.2 -12 21 KUI 57 Kappa Crt. 11 27.2 -15 39 HU 462 P = 48.5yr., a = 0.45", motion retrograde. 11 27.7 +46 18 STF 1541 Proper motion of B +004 -097. 11 27.9 +02 51 STF 19 Tau Leo. B is BD+03@2505. 11 28.1 -61 25 COO 269 A is an Algol-type system, MN Cen. 11 28.6 -42 40 BSO 6 A is a spectroscopic binary. 11 29.1 +39 20 STF 1543 57 UMa. A is a spectroscopic binary. 11 29.2 -17 21 H 112 H IV 112. S 627. 11 29.6 +11 38 HJ 2572 Proper motion of B +023 -031. 11 29.6 -24 28 JC 16 Proper motion of B -046 +012. 11 30.1 +29 58 STT 111 LDS 5730. B is BD+30@2164. The primary is the eclipsing pair AW UMa, P = 0.44d. Proper motion of B -092 -204. 11 30.3 +81 02 STF 1539 B is BD+81@370. Proper motion of B +038 +025. 11 30.8 +41 17 STT 234 P = 87yr., a = 0.39", motion direct. Also a spectroscopic binary, P = 7.40d. 11 30.8 -58 49 FIN 187 Spectrum of B: F. 11 31.3 +59 42 STF 1544 B is a spectroscopic binary. Proper motion of B +015 +008. 11 31.7 +14 22 STF 1547 88 Leo. Proper motion of B -328 -188. 11 31.8 -59 27 HJ 4445 Omicron (1) Cen. A semiregular variable. 11 32.0 -52 27 HJ 4446 B is CD-51@5787. 11 32.1 -63 57 HJ 4447 B is CPD-63@1914. 11 32.2 +36 15 HU 1134 The orbit is edge-on: P = 80yr., a = 0.20". 11 32.3 +61 05 STT 235 P = 73.0yr., a = 0.81", motion direct. 11 32.3 -29 16 H 96 H III 96. Proper motion of B -003 +154. 11 32.5 +53 02 HJ 2574 C is a nebula, NGC 3718. Proper motion of B -055 -018. 11 32.6 +24 19 STF 1549 Proper motion of B -007 -070. 11 33.0 -31 51 HJ 4449 Xi Hya. 11 34.7 +16 48 STF 1552 90 Leo. B is a spectroscopic binary. 11 35.0 +33 48 A 2159 Round 1952, 1953, 1956 with 82-inch. 11 35.2 -47 22 RST 548 A is the semiregular variable V763 Cen. 11 35.3 +70 48 STF 1551 Proper motion of B +002 -026. 11 35.8 -63 01 RST 3746 Lambda Cen. 11 36.3 +27 47 STF 1555 A is a spectroscopic binary. A premature visual orbit has been computed. 11 36.3 +12 08 STF 1556 Proper motion of B -028 +031. 11 36.6 +56 08 STF 1553 Proper motion of B -176 -088. 11 36.8 -12 21 BU 456 P = 365yr., a = 1.02", motion direct. 11 37.0 -38 58 DUN 113 B is CD-38@7231. Proper motion of B +055 -008. 11 37.4 +47 28 KU 39 A is a BY Dra-type variable, and also a spectroscopic binary. A premature visual orbit has been computed. 11 37.6 -16 56 HJ 1192 Proper motion of B -059 -016. 11 37.8 -48 55 HJ 4459 B is CD-48@6669. 11 38.3 -63 22 I 422 Light and radial velocity variable. 11 38.7 +45 07 STF 1561 B is a spectroscopic binary. Proper motion of B -578 -007. 11 38.7 -13 12 KUI 58 Iota Crt. 11 39.3 +06 10 HJ 2580 Proper motion of B -042 -002. 11 39.5 -65 24 B 1705 A spectroscopic binary. 11 39.6 +19 00 STF 1565 B is BD+19@2482. Proper motion of B -041 -005. 11 39.8 -63 29 BSO 7 B is CPD-62@2205. Proper motion of B -005 +009. 11 40.0 -38 06 DUN 114 Proper motion of B -047 -026. 11 40.1 -03 26 GAU 13 Gauchet calls this HJ 186, but it seems to be another pair. 11 41.0 -62 42 B 799 A is the Cepheid UZ Cen. 11 41.1 +34 12 STT 61 UMa. 11 41.4 +58 55 ES 2638 B is BD+59@1396. Proper motion of B -215 -042. 11 41.6 +31 45 BNU 62 UMa. B is BD+32@2178, proper motion +001 -088. 11 42.4 +00 02 HJ 1194 Proper motion of B -046 +021. 11 43.1 -36 01 I 1546 Position angles uncertain, too close. Needs speckle. 11 43.3 +00 46 STF 1568 Proper motion of B -014 +001. 11 43.4 +22 45 POU 3110 Heintz believes HJ 2581 to be identical. 11 43.7 +13 31 HJ 2583 B is BD+14@2427. Proper motion of B -005 -003. 11 43.8 +24 23 HJ 509 Proper motion of B +018 -007. 11 43.8 +18 31 BRT 2412 Proper motion of B -157 -004. 11 44.1 -04 48 RST 5524 Obviously in rapid motion, but the measures are insufficient to define the nature of the motion. 11 44.5 +14 37 HJ 4469 Proper motion of B -032 +012. 11 44.6 -49 25 RST 3558 RST 3558a. P = 32.35yr., a = 0.28", motion direct. 11 44.8 +28 26 ES 435 Proper motion of B -038 -006. 11 44.8 +11 23 J 3234 Proper motion of B +044 -147. 11 45.5 +45 36 STF 1570 Proper motion of B +008 +029. 11 45.6 -66 44 HJ 4471 Lambda Mus. 11 45.9 +11 22 J 1017 Single 1933 and 1953. The measure in 1910 doubtful. No certain measures since. 11 46.4 +09 04 STF 1571 Proper motion of B +009 -027. 11 46.7 -40 29 LDS 6248 Proper motion -1.545 +0.385. 11 47.5 +20 02 SHJ 130 B is BD+20@2651. Proper motion of B 000 -012. 11 47.9 +08 15 CHR 134 4 Vir. 11 48.0 +20 13 STF 7 93 Leo. A is a spectroscopic binary and light variable, spectrum composite; A7V+G5III-IVe. B is BD+21@2357. Proper motion of B -155 +005. 11 48.0 -08 38 STF 3074 Proper motion of B +074 -050. 11 48.4 -10 19 H 115 H VI 115. B is BD-09@3368. 11 48.6 +14 17 BU 603 P = 134yr., a = 0.71", motion retrograde. 11 48.7 -61 34 R 176 R 176a. 11 49.1 +14 34 BU 604 Beta Leo. Possibly variable. 11 49.2 +67 20 STF 1573 Proper motion of B +027 -003. 11 50.7 +01 46 STT Beta Vir. Proper motion of C -066 -013. 11 51.0 -05 20 MCA 36 A spectroscopic binary and suspected occultation binary now resolved by speckle interferometry. 11 51.2 +33 22 ARG 101 B is BD+34@2263. 11 51.8 -03 35 J 1581 Probably variable (Jonckheere). 11 51.8 -05 46 CHR 36 This is the variable TY Vir. 11 52.0 +78 56 HJ 1200 Proper motion of B +050 -006. 11 52.0 +48 05 HU 731 P = 196yr., a = 1.10",motion retrograde in a highly- inclined orbit. 11 52.0 +08 50 STF 1575 B is BD+09@2552. Proper motion of B +020 -058. 11 52.4 +07 33 STF 3075 Proper motion of B -001 -014. 11 52.8 +15 26 SHJ 132 Proper motion of B +030 -060. 11 52.9 +30 50 STF 1576 Proper motion of B -074 +026. 11 52.9 -33 54 HJ 4478 Beta Hya. A is an Alpha CVn-type variable. 11 53.2 -15 40 A 2579 P = 175yr., a = 0.29", motion retrograde. 11 53.3 +83 11 LDS 1743 B is BD+83@342. 11 53.3 +20 19 STF 1577 Proper motion of B -006 +007. 11 53.7 +73 45 BU 794 P = 77.2yr., a = 0.39", motion direct. 11 54.1 +71 55 A 75 P = 82.3yr., a = 0.267", motion retrograde. 11 54.1 +24 41 HJ 512 Proper motion of C +001 -004. 11 54.5 +19 25 STT 112 B is BD+20@2659. Proper motion of B -443 -014. 11 54.7 -56 19 BRT 3166 Perhaps CPD-55@4708. 11 55.0 -62 35 BSO 20 B is CPD-61@2779. Proper motion of B -001 -015. 11 55.1 +46 29 A 1777 65 UMa. The primary is the eclipsing binary DN UMa, P = 1.73d. AB: P = 115yr., a = 0.22", motion direct. 11 55.5 +72 29 MLR 426 Duplicity uncertain. 11 55.6 +16 54 KU 41 Proper motion of B +019 -017. 11 55.7 +15 39 H 13 H VI 13. 95 Leo. All stars in the field are much more than 90" away. A is a spectroscopic binary. 11 56.0 +21 59 STF 1582 Proper motion of B -057 -008. 11 56.1 +45 33 STF 1581 A is a RR Lyrae-type variable. B also variable? 11 56.3 -45 46 LDS 373 B is CD-45@7400. 11 56.6 -04 37 STF 1584 B is BD-03@3206. 11 56.7 -32 16 DUN 116 B is CD-31@9364. 11 57.8 +45 18 A 1778 A may be variable. 11 58.9 -25 55 I 510 Too close. Duplicity doubtful, and/or rapid motion. Needs speckle. 11 59.2 -62 47 COO 133 Proper motion of B +032 -002. 11 59.4 -42 19 HJ 4485 A is CPD-41@5660. B is CPD-41@5659. 11 59.6 -78 13 HJ 4486 Epsilon Cha. 12 00.1 +70 39 STT 242 C is BD+71@595 according to ADS, but A and C may be reversed. 12 00.2 +87 00 STF 1583 B is BD+87@100. 12 00.2 +36 44 STT 114 B is BD+37@2239. Proper motion of B -014 -021. 12 01.5 -00 23 STF 1591 B is BD+00@2877. Proper motion of B +003 -011. 12 01.6 +70 51 STF 1590 Proper motion of B -018 +007. 12 01.8 -34 39 I 215 A premature orbit has been computed. The motion is nearly rectilinear, but the sizable proper motion proves the physical nature. 12 01.9 +00 06 STT 116 B is BD+00@2881. Proper motion of B +013 -014. 12 02.1 +43 03 FOR 1 67 UMa. A is a Delta Scuti-type variable, DP UMa. Position of B (+43@2182): 12 02.5 +43 05. 12 02.3 +72 22 STF 1588 Proper motion of B -008 +015. 12 02.3 -85 38 HJ 4490 B is CPD-84@372. Proper motion of B -035 +022. 12 03.0 -63 19 CPO 55 Theta (1) Cru. A is a spectroscopic binary. 12 03.5 -36 55 HJ 4499 Proper motion of B -047 -066. 12 03.6 -39 01 SEE 143 89 Cen. P = 109yr., a = 0.66", motion retrograde. 12 03.8 -44 07 HJ 4491 B is CD-43@7447. Proper motion of B +105 +020. 12 04.0 +64 29 STI 739 Proper motion of B +001 +002. 12 04.0 +03 21 ENG 46 B is BD+04@2568. Proper motion of B +057 -572. 12 04.2 +24 07 A 682 A close approach took place from about 1960-1975. 12 04.3 +21 28 STF 1596 2 Com. A spectroscopic binary. Proper motion of B +028 +010. 12 04.3 +07 24 STF 1595 Proper motion of B +002 -021. 12 04.3 -21 02 BU 458 B is BD-20@3568. 12 04.7 -05 46 RST 4492 A is the semiregular variable RX Vir. 12 04.8 -40 03 RST 1641 CPD-39@5381. 12 04.8 -62 00 DUN 117 B is CPD-61@2935. Proper motion of B -020 +011. 12 04.8 -67 04 DON 1095 CD-66@1160. 12 04.9 +09 10 STF 1597 B is BD+09@2580. Proper motion of B -021 -006. 12 05.1 -61 11 FIN 421 The composite spectrum is unlikely to refer to B. 12 05.4 -26 36 RST 2777 Motion direct, companion optical. 12 05.6 +68 48 STF 1599 Proper motion of B -002 -025. Proper motion of D -027 -004. Proper motion of E -053 -004. Djurkovic measured component Ee: 70@, 0.2", 8-8, but van den Bos found this round in 1958. 12 05.6 +51 56 STF 1600 Proper motion of B -007 -013. 12 05.9 -49 51 HJ 4494 CPD-49@4827. 12 06.0 +68 42 STF 3123 P = 122.3yr., a = 0.296", motion retrograde. C is probably physical. 12 06.1 +70 22 A 76 B is BD+71@603. 12 06.2 -20 02 B 1714 A rapid binary, angles and period uncertain. 12 06.4 -48 58 BRT 805 CPD-48@4508. 12 06.4 -65 43 FIN 367 Composite spectrum; G8-K0III+A3. 12 06.6 -37 52 HJ 4500 B is CD-37@7665. 12 06.9 -64 37 HJ 4501 Eta Cru. A is a spectroscopic binary. 12 07.1 +69 05 STF 1602 The A component is a spectroscopic triple, P = 3.87d and 6.5yr. 12 08.1 +55 28 STF 1603 B is BD+56@1569. Proper motion of B -181 -029. 12 08.4 -50 43 JC 2 Delta Cen. A is a Cepheid. B is CD-49@6813. 12 09.4 -34 09 RST 2782 Spectrum: G5/6III/IV. 12 09.5 -11 51 STF 1604 AB: Mt. Wilson spectral types are G2 and K8. A is a spectroscopic binary, and slightly variable. 12 09.7 +01 54 BUP 138 10 Vir. 12 10.1 -43 34 CPO 56 B is CD-42@7455. Proper motion of B -050 +040. 12 10.5 +16 49 CHR 135 3 Com. 12 10.5 -02 14 STF 1605 Proper motion of B +000 -034. 12 10.8 +39 53 STF 1606 P = 327yr., a = 0.77", motion retrograde. 12 11.0 +81 43 SHJ 136 BDS 6074, STT (App) 118 probably same star. B is BD+82@357. Proper motion of B +012 +028. 12 11.4 +43 34 LDS 4186 B is BD+44@2169. 12 11.4 -60 57 RST 4493 Spectral type B5? 12 11.5 +53 25 STF 1608 Mt. Wilson spectral types are K2 and G9. Proper motion of B -161 -123. 12 11.7 +50 50 STF 1609 Proper motion of B -012 +018. 12 11.9 +20 24 HJ 2601 Proper motion of B 000 -009. 12 12.6 +10 46 STF 1612 Proper motion of B -040 +024. 12 12.9 -44 42 HRG 75 Proper motion of B -019 +007. 12 12.9 -44 54 HJ 4507 B is CD-44@7860. Proper motion of B -014 +007. 12 13.1 +67 04 STF 1614 Proper motion of B -012 +007. 12 13.7 +78 26 HU 891 Proper motion of B -010 -089. 12 14.0 -45 43 RMK 14 A is a spectroscopic binary. 12 14.1 +32 47 STF 1615 B is a spectroscopic binary. 12 14.3 +11 49 HU 1137 A is a W UMa-type system, AH Vir. 12 14.3 -05 43 HJ 203 A is the Delta Scuti-type variable FG Vir. 12 14.5 +08 47 STF 1616 The declination differences between A and BD+09@2600 have been measured. See ADS. Proper motion of B +047 -127. 12 14.8 -55 47 HJ 4508 B is CPD-55@4937. 12 15.1 +09 59 STF 1618 Proper motion of B -015 -006. 12 15.1 +07 32 STF 1617 Proper motion of B -007 +042. 12 15.1 -07 15 STF 1619 C is BD-06@3533. 12 15.2 -10 19 BUP 139 Proper motion of A +036 -1016. 12 15.4 +57 02 BLL 29 Delta UMa. 12 15.5 -31 06 RST 1658 P = 66yr., a = 0.68", motion direct. 12 16.0 +48 07 HU 736 P = 218yr., a = 0.28", motion retrograde. 12 16.0 +05 38 STF 1621 P = 875yr., a = 2.93", motion direct. 12 16.1 +40 40 STF 1622 2 CVn. A is a spectroscopic binary. Proper motion of B +021 -027. 12 16.2 +80 08 STF 1625 B is BD+80@380. Proper motion of B +027 -001. 12 16.2 +04 43 STF 1623 Proper motion of B -139 -005. 12 16.5 +41 49 HJ 1215 Proper motion of B -039 -009. 12 16.5 +33 04 CHR 37 A Delta Scuti-type variable and long-period (1300d) spectroscopic binary. 12 17.5 +06 36 BU 796 Single 1944-5, 1952-60. 12 18.2 -03 57 STF 1627 B is BD-03@3262. Proper motion of B -004 +024. 12 18.2 +05 15 HJ 2609 C is a nebula, HJ 1178. 12 18.2 -03 57 STF 1627 B is BD-03@3262. 12 18.2 -52 18 I 1220 Too close since 1928. Last attempted in 1959. Needs speckle. 12 18.4 -64 00 HJ 4512 Zeta Cru. 12 18.7 +11 48 STF 1628 BDS 6116, HJ 1216 same star. Proper motion of B -001 -029. 12 19.0 -33 18 HJ 4513 B is CD-32@8628. 12 19.9 -00 40 MCA 37 Eta Vir. A spectroscopic and occultation binary now resolved by speckle interferometry: P = 13.1yr., a = 0.136", motion direct. 12 20.1 +13 51 BU 27 A is variable. 12 20.2 +37 54 STF 1632 Proper motion of B -059 +013. A is a spectroscopic binar binary. 12 20.3 +03 19 BUP 141 16 Vir. 12 20.6 -22 13 BU 1245 Zeta Crv. A is a spectroscopic binary. 12 20.7 +27 03 STF 1633 Proper motion of B +035 -126. 12 20.7 +17 48 HO 52 11 Com. 12 21.1 -11 29 STF 1635 Proper motion of B -027 -024. 12 21.6 -27 16 B 227 Motion direct. 12 22.1 -67 31 HDO 215 Zeta (2) Mus. 12 22.2 +58 05 WNC 4 Proper motion of B -026 +068. 12 22.5 +25 51 SHJ 143 12 Com. A is a spectroscopic binary. Spectrum composite: G0III-IV+A3V. Proper motion of C -028 -008. 12 22.5 +05 18 STF 1636 17 Vir. B may be variable. Proper motion of B -172 -047. 12 23.9 -03 03 HJ 209 Proper motion of B -012 -025. 12 24.0 -62 06 COO 137 Spectrum A0/2+K1/2III 12 24.4 +25 35 STF 1639 P = 678yr., a = 1.30", motion retrograde. 12 24.4 -52 50 HJ 4520 B is CPD-52@5564. 12 24.6 +37 44 STF 1641 AB: Proper motion of B +008 +017. 12 24.7 +02 25 AG 177 Proper motion of B -051 +053. 12 24.8 -28 27 BRT 2993 CPD-27@4502. 12 24.9 -58 07 BSO 8 Spectrum F8/G2IV/V+A. 12 25.5 -69 29 HJ 4522 Proper motion of B -043 -101. 12 26.6 -63 06 DUN 252 Alpha (1) Cru. Spectroscopic binary. Common proper motion with HR 4729 and 4731, so that there are at least five components in the system. 12 26.9 -37 28 HJ 4510 B is CD-36@7850. BC: C is CPD-36@5498. Proper motion of C -029 -025. 12 27.2 +27 01 STF 1643 A premature orbit has been computed. 12 27.2 -19 58 S 637 B is BD-19@3492. 12 27.3 +07 14 FOX 175 Proper motion of B -119 +081. 12 27.4 +07 23 STF 1644 Proper motion of B +027 -012. 12 27.4 -28 43 B 228 P = 46yr., a = 0.16", motion direct. 12 28.1 +44 48 STF 1645 Alternative spectra F5+K. (Mt. Wilson F8+G0). Proper motion of B -182 -005. 12 28.1 -60 02 HJ 4524 B is CPD-59@4236. 12 28.7 -71 29 LDS 410 Proper motion -419 +1091. 12 28.9 +25 55 STF 21 A is an Alpha CVn-type variable, AI Com. B is a spectroscopic binary. 12 29.1 +31 23 STT 251 P = 600yr., a = 0.61", motion direct. 12 29.9 -16 31 SHJ 145 Delta Crv. B is BD-15@3481. Proper motion of B -206 -129. A may be variable. 12 30.0 +51 32 BUP 143 7 CVn. C is BD+52@1630. Proper motion of C +023 -004. 12 30.1 -13 24 BU 28 P = 162yr., a = 1.38", motion direct. 12 30.4 +36 08 HJ 519 Proper motion of B -013 -015. 12 30.6 +03 31 STF 1648 Proper motion of B -057 -008. 12 30.7 +75 18 DOO 55 Proper motion of B +001 -013. 12 31.0 -53 12 HJ 4526 B is CPD-52@5648. 12 31.1 -05 19 A 3084 Too close 1935, 1958, and 1986. 12 31.2 +01 20 SHJ 146 B is BD+02@2551. 12 31.2 -57 07 DUN 124 Gamma Cru. A variable? B is CPD-56@5274. Proper motion of B +010 -018, spectrum A3V. 12 31.6 -11 04 STF 1649 B is BD-10@3486. Proper motion of B -048 +001. Mt. Wilson spectral types A3, F2. 12 32.1 +74 49 STF 1654 Proper motion of B -015 -001. 12 32.3 +20 00 HU 571 Possible quadrant reversal about 1920-1930. 12 32.5 +21 06 STF 1652 Proper motion of B -024 -001. 12 33.4 +32 02 STF 1653 Proper motion of B +004 -015. 12 33.5 +10 12 HJ 212 Proper motion of B -010 -030. 12 33.5 +09 01 REU 1 Wolf 424. P = 16.2yr., a = 0.76", motion retrograde. However, this interpretation is subject to some contro- versy. The pair also exhibits flares. 12 33.6 +38 37 STF 1656 B is BD+39@2534. 12 33.7 +41 21 BNU Beta CVn. A spectroscopic binary and Beta CVn-type variable now probably resolved by speckle inter- ferometry. 12 34.9 +22 38 WRH 12 23 Com. A spectroscopic binary. 12 35.1 +18 23 STF 1657 24 Com. B is a spectroscopic binary. Proper motion of B -006 +022, spectrum A9Vm. 12 35.1 +07 27 STF 1658 AB: Proper motion of B +180 -095. 12 35.8 +56 35 STF 1662 Proper motion of B 000 +002. 12 36.2 -46 50 RST 5526 Motion retrograde. 12 37.2 -69 08 DON 541 Alpha Mus. Variable. 12 38.0 +44 44 HJ 1219 Proper motion of B +032 -074. 12 38.3 +03 30 BAL 2854 Proper motion of B -006 -012. 12 38.3 -58 07 HJ 4534 B is CPD-57@5606. 12 38.7 -04 22 S 639 B is BD-03@3330. Proper motion of B -026 -036. 12 39.1 -58 16 R 205 B is CPD-57@5611. 12 39.2 +14 20 STF 1666 Spectrum of A composite; A3+G. Proper motion of B -010 +031. 12 39.2 -08 00 ENG 47 Chi Vir. B is BD-07@3454, proper motion -025 -016. Spectrum of A: K2III-IIIbCN1. 12 39.2 -40 22 B 1215 P = 66yr., a = 0.24", motion direct. 12 39.6 -37 17 DAW 63 P = 57yr., a = 0.33", motion direct. 12 39.8 +74 41 HJ 2618 Proper motion of B 000 +016. 12 41.3 -13 01 STF 1669 Both A and B are spectroscopic binaries, with periods of 44.4 and 1.46d. Both may also be variable. Proper motion of B -117 +026. 12 41.5 -48 58 HJ 4539 Gamma Cen. P = 84.5yr., a = 0.93", motion retrograde. 12 41.6 +10 26 H 81 H VI 81. 27 Vir. A is the Delta Scuti-type variable GG Vir, and is also a spectroscopic binary. 12 41.7 -01 27 STF 1670 Gamma Vir. P = 169yr., a = 3.70", motion retrograde. One component is a suspected variable. 12 42.0 +06 48 BU 924 31 Vir. 12 42.0 -22 02 DON 547 CPD-21@5405. 12 42.0 -41 13 CPO 351 CPD-40@5868. 12 42.2 +26 22 A 1851 P = 61.1yr., a = 0.40", motion direct. 12 42.9 +05 16 A 1602 Single 1935, 1952, 1956. 12 43.1 -72 47 HJ 4540 Proper motion of B +004 -050. 12 43.3 -33 41 I 1558 CPD-33@3294. Spectrum: G8IVCNIII. 12 44.0 +21 10 STT 253 Proper motion of B -042 +029. 12 44.0 +03 56 A 1603 B may be variable. 12 44.1 +35 46 HO 256 Spectrum: A7/A8V/F2/3. 12 44.3 -55 53 R 206 B is CPD-55@5202. 12 44.5 +34 25 STF 1675 Proper motion of B -047 -044. 12 44.9 -52 45 HJ 4546 B is CPD-52@5846. Proper motion of B +028 +008. 12 45.3 -03 53 STF 1677 B is BD-03@3348. Proper motion of B -033 +005. 12 45.4 +14 22 STF 1678 B is BD+15@2503. 12 45.6 -60 59 HJ 4547 Iota Cru. 12 46.0 +49 49 STF 1679 Proper motion of B +017 +011. 12 46.3 -68 06 R 207 Beta Mus. P = 383yr., a = 1.74", motion direct. A has variable radial velocity. 12 46.4 +09 32 STT 33 Vir. B is BD+10@2467. Proper motion of B -095 -026. 12 46.4 -56 29 HJ 4548 B is CPD-55@5216 and is a suspected variable. Proper motion of B -019 -007. 12 46.7 -19 01 B 2540 Too close 1951, 1953, 1959. 12 47.2 +11 57 BUP 145 34 Vir. 12 47.2 -41 05 WG 155 CPD-40@5908. 12 47.7 -59 41 I 362 Beta Cru. A is a Beta CMa-type variable. 12 47.9 +32 08 SEI 533 Proper motion of B -051 -044. 12 48.2 -24 48 HJ 4551 Proper motion of B -321 +145. 12 48.3 -67 08 HJ 4550 Proper motion of B -037 -027. 12 48.5 +81 34 LDS 1758 B is BD+82@376. 12 49.1 +42 13 ES 2643 B is BD+43@2262. 12 49.1 -51 25 RST 5368 CPD-50@5488. 12 49.2 +83 25 STF 1694 B is +84@289 and is a spectroscopic binary, spectrum A0V+A2V, proper motion -023 +019. 12 49.3 +27 33 CHR 179 30 Com. A is a spectroscopic binary, now probably resolved by speckle interferometry. 12 49.6 +03 49 STF 1681 Proper motion of B -075 +005. 12 49.7 +01 11 ENG 50 B is BD+02@2584. 12 50.7 +20 32 HU 640 P = 117yr., a = 0.59", motion direct. 12 51.2 -46 52 HJ 4552 B is CD-48@8210. 12 51.4 -10 20 STF 1682 B is BD-09@3568. One component variable? 12 51.7 -33 28 I 1561 Spectrum: Fm delta Del. 12 51.9 +34 47 HJ 523 Proper motion of B -017 -051. 12 51.9 +19 10 STF 1685 Proper motion of B -070 +007. 12 52.0 -26 48 B 234 P = 122yr., a = 0.36", motion direct. 12 52.2 +17 04 STF 23 32 Com. B is BD+17@2553. Proper motion of B +046 -042. 12 53.0 +15 02 STF 1686 Proper motion of B -018 +024. 12 53.2 -03 33 CHR 38 38 Vir. 12 53.3 +21 15 STF 1687 35 Com. P = 510yr., a = 1.42", motion direct. C is physical, and is in slow direct motion. 12 54.0 +55 58 BLM Epsilon UMa. An Alpha CVn-type variable and eclipsing system. 12 54.0 -18 02 S 643 B is BD-17@3725. Proper motion of B -018 +002. 12 54.2 +52 50 BEM 2 Position corrected by Heintz. 12 54.6 -57 11 DUN 126 Mu (1) and (2) Cru. Proper motion of B -023 -008. B is variable, spectrum B5Vne. 12 55.0 +58 10 STF 1691 AB: Proper motion of B -004 -062. 12 55.0 -85 07 RST 2819 Iota Oct. 12 55.4 +69 53 A 1092 P = 58yr., a = 0.22", motion retrograde. 12 55.5 +11 30 STF 1689 Proper motion of B -080 +026. 12 55.6 +03 24 BUP 146 Delta Vir. 12 56.0 +38 19 STF 1692 Alpha CVn. Both components are spectroscopic binaries. Prototype of the Alpha CVn-type variables. Proper motion of B -226 +060, spectrum F0V. 12 56.3 +54 06 STF 1695 A spectroscopic binary, P = 5.13d. Proper motion of B -016 +032. 12 56.4 -30 07 HJ 4558 B is CD-29@10020. 12 56.7 +45 37 STT 257 Proper motion of B -034 -021. 12 56.7 +07 01 STF 1693 Proper motion of B +003 -039. 12 56.7 -47 41 I 83 P = 294yr., a = 0.70", motion direct. 12 57.5 +18 42 BGH Proper motion of B -234 +109. 12 57.6 +35 14 LDS 6271 Spectra dM1.5e and dM3.5e. Starspots exist on A, and it is also a flare star. 12 57.9 +49 48 HU 641 Round 1950, 1953, 1956, 1957. Apparent rapid motion. A premature orbit has been calculated. 12 58.2 -54 11 COO 143 Proper motion of B -032 -018. 12 58.4 +58 22 HJ 2628 B is BD+59@1476. Proper motion of B +013 -001. 12 58.5 +38 17 STF 1702 B is BD+39@2587. 12 58.5 -46 18 DON 568 CPD-45@6129. 12 59.3 +06 30 STF 1701 Proper motion of B -031 -014. 12 59.5 -48 32 HJ 4562 B is CD-47@8001. 12 59.7 -03 49 CHR 39 44 Vir. Rapid binary. 12 59.8 -55 55 DUN 127 B is CPD-55@5317. 13 00.2 -23 55 I 1225 Measures uncertain, too close. Needs speckle. 13 00.3 +30 47 BU 1081 37 Com. 13 00.3 -64 13 RST 5372 Spectrum: F3/6IV/V+A. 13 00.4 +35 45 HU 1141 Variability has been reported. 13 00.6 -03 22 AGC 5 46 Vir. 13 00.7 +73 43 HJ 2633 Proper motion of B -070 -116. 13 00.7 +56 22 BU 1082 78 UMa. P = 107yr., a = 1.28", motion direct. 13 00.8 +14 23 STF 1705 Proper motion of B -022 -071. 13 01.5 -58 08 COO 146 Spectrum: A5/7+A1/2V. 13 02.1 +07 17 STF 1708 Proper motion of B -118 +027. 13 02.2 +10 58 BUP 147 Epsilon Vir. Optical. 13 03.3 -59 36 COO 147 Spectrum: F5IV/V+A/F. 13 03.5 +09 28 STF 1712 Proper motion of B -045 +015. 13 03.9 -03 40 BU 929 48 Vir. 13 04.2 +19 24 STF 1715 Proper motion of B -034 -019. 13 04.4 -13 16 HU 642 P = 108yr., a = 0.34", motion retrograde. Possibly an ambiguous case. 13 05.2 +09 12 GEL Wolf 472,3. 13 05.4 -57 35 I 914 Spectrum of secondary: A/F. 13 05.5 +50 59 HU 643 Proper motion of B -010 -023. Proper motion of C +030 -018. 13 05.8 -31 11 BRT 2997 CD-30@10320? 13 06.2 +29 02 BU 1083 BC: Single in 1958 (van den Bos). Only two attempts since 1901, in 1958, with negative results. 13 06.4 +76 18 HJ 2644 B is BD+77@501. 13 06.4 +21 09 CHR 150 39 Com. 13 06.7 -21 11 HJ 2637 B is BD-20@3775. Proper motion of B +020 +002. 13 06.8 +28 36 AG 344 Proper motion of B -030 +010. 13 06.8 +26 57 L 12 Round 1945 through 1969. 13 06.9 -49 54 DUN 128 Xi (2) Cen. A is a spectroscopic binary. 13 07.3 +00 35 STF 1719 Proper motion of B -086 -128. 13 07.4 -59 52 R 213 Spectrum composite; B9IV+F8-G2. 13 07.5 -62 07 HJ 4568 B is CPD-61@3460. 13 07.6 +26 29 BUP 148 B is BD+27@2217. Proper motion of B -103 +017. 13 07.6 -61 44 R 212 Proper motion of B +035 +005. 13 07.7 +24 01 STT 259 B is BD+24@2540. Proper motion of B -267 +146. 13 08.1 -65 18 RMK 16 Theta Mus. Wolf-Rayet binary, second brightest in the sky. 13 08.4 +62 36 MLB 412 Heintz corrects the declination. 13 08.5 +01 07 STF 1721 Proper motion of B -003 -005. 13 08.5 -02 41 S 647 Proper motion of B -030 +042. 13 09.1 +21 27 HU 572 P = 134yr., a = 0.40", motion retrograde. 13 09.2 +08 48 A 1786 Proper motion of B +022 -001. 13 09.5 -13 13 BRT 2732 13 04.3 -12 47 (Mason) may be same star. 13 09.7 +38 32 BU 608 BC: 15 CVn. Optical with A at 13101+3830. 13 09.8 +62 14 STT 121 Proper motion of B -037 -023. 13 09.9 +31 22 STF 1727 Proper motion of B -029 -067. 13 09.9 -05 32 MCA 38 Theta Vir. Also a long-period spectroscopic binary. H 50 Aa-C: H III 50. 13 10.0 +17 32 STF 1728 Alpha Com. P = 25.8yr., a = 0.668", inclination 90 degrees. 13 10.1 +38 30 STF 24 17 CVn. Optical with BC, BU 608, at 13097+3832. 13 10.2 +73 58 STT 262 B is BD+74@524. Prpoer motion of B -035 +011. 13 10.3 -34 47 B 2015 Rapid direct motion. 13 11.2 +30 50 A 1359 B not seen in 1957 (82-inch). Single 1959 (15-inch). 13 11.5 -35 08 HJ 4571 B is CD-34@8707. Proper motion of B -016 -012. 13 11.7 -26 33 FIN 305 P = 19yr., a = 0.12", motion retrograde. 13 11.7 -32 16 HJ 4572 Proper motion of B -071 +011. 13 11.9 +27 53 STT Beta Com. Possibly a long-period spectroscopic binary. 13 11.9 -20 38 DON 588 CPD-19@5377. 13 12.1 -16 12 HJ 2645 53 Vir. AC: Not found in 1908 (Burnham). 13 12.3 -59 55 SEE 170 P = 27yr., a = 0.18", motion direct. The A component is a Beta Lyrae-type system. I 424 AB-C: C is also physical. 13 12.4 -49 37 CPO 364 B is CD-48@8008. 13 12.5 -34 45 LDS 436 B is CD-34@8719. 13 12.9 -59 49 COO 152 A may be a spectroscopic binary. 13 13.1 +18 01 S 648 B is BD+18@2703. Proper motion of B -010 -032. 13 13.2 -02 33 STF 1731 Proper motion of B -159 -017. 13 13.4 -18 50 SHJ 151 54 Vir. Both components are spectroscopic binaries. 13 13.4 -50 42 I 1227 Fairly rapid retrograde motion. 13 13.5 +67 17 STF 25 AB: Spectrum K2III+K2III. Position of C: 13 13.0 +67 19. 13 13.7 +29 49 HO 55 Single in 1958 (van den Bos, Couteau). Failure to see the companion is probably due to the large magnitude difference. 13 13.7 -01 34 BAL 549 Proper motion of B -013 -001. 13 14.1 -65 55 BRT 2003 CPD-65@2212 or 2213. 13 14.5 -24 17 FIN 297 P = 61yr., a = 0.16", motion direct. 13 14.7 -63 35 MLO 3 Spectroscopic binary. 13 15.2 -67 54 DUN 131 Eta Mus. The primary is a spectroscopic binary and a possible eclipsing system. 13 16.4 +42 02 HJ 1230 HJ observes HJ 1230: 1828 290@ 12" 11-11. 13 16.8 +09 25 KUI 62 59 Vir. 13 16.9 -34 36 I 1567 P = 42yr., a = 0.30", motion retrograde. 13 17.5 -00 41 FIN 350 P = 9.05yr., a = 0.080", motion direct. 13 18.4 +54 20 HJ 2649 Proper motion of B -047 +022. 13 18.4 -18 19 H 90 61 Vir. H VI 90. Proper motion of A -1070 -1065. B is BD-17@3815. 13 18.9 -23 10 SMY 3 Gamma Hya. 13 19.0 -26 37 UPT 2 Proper motion of B -045 -002. 13 19.8 +47 47 HU 644 P = 48.9yr., a = 1.47", motion retrograde in a highly- inclined orbit. 13 19.9 -27 48 B 247 Spectrum: Fm delta Del. 13 20.3 +17 46 A 2166 P = 11.15yr., a = 0.120", motion direct. 13 21.7 +15 42 FOX 177 Proper motion of B -066 -005. 13 21.8 +05 50 STF 1735 Proper motion of B -044 -054. 13 22.3 -11 37 LDS 439 Proper motion of B +100 -062. 13 22.5 -22 57 ARG 26 B is BD-22@3573, spectrum G1/2V. Proper motion of B -029 +008. 13 22.6 -60 59 FIN 208 Too close, measures uncertain. One component is the variable V790 Cen. 13 22.7 +35 56 HJ 530 Proper motion of B +023 +020. 13 22.8 -13 11 H 119 H IV 119. B is BD-12@3801. A is a spectroscopic binary, called "mild Am" by Bidelman. 13 22.9 +89 32 HJ 3154 2000 position deduced from 1830: 22 47.4 +89 28. 13 22.9 -72 09 B 1736 Spectroscopic binary. 13 23.5 +29 14 HO 260 P = 229yr., a = 2.14", motion direct. 13 23.7 +02 43 STF 1740 B is BD+03@2766. Proper motion of B +005 +200. 13 23.7 -00 43 A 2489 A premature orbit has been computed. 13 23.8 +38 31 HU 1259 Distance < 0.1" with 82-inch in 1956 (van Biesbroeck). Single with smaller telescopes 1963-1992. 13 23.9 +54 56 STF 1744 Zeta UMa. A is a spectroscopic binary (the first discovered), P = 20.54d. B is also a spectroscopic binary, P = 175.6d, spectrum A1m or A1/A2/A7, Proper motion +115 -033. Also, common proper motion with 80 UMa and other members of the Ursa Major stream. 13 24.0 -20 55 BU 610 Spectrum: K1/2III/IV. 13 24.2 -01 59 GLP 9 B is BD-01@2813. 13 24.2 -02 06 STF 1741 Proper motion of B +006 -034. 13 24.6 -51 30 I 1231 Too close after 1927. Needs speckle. 13 25.2 -11 10 BUP 150 Alpha Vir. A is an Alpha CVn-type variable and a spectroscopic binary, spectrum B1III-IV+B2V. It has been resolved by intensity interferometry. 13 25.3 +75 59 STT 267 Position angles scattered, mostly near 150@. Quadrant uncertain. Probably in rapid motion. 13 25.3 +40 28 HJ 1231 This is a measure of A and BD+41@2392. Proper motion of BD+41@2392 +016 000. 13 25.3 +10 33 HJ 227 Proper motion of B -037 +004. 13 25.8 +44 30 A 1609 P = 44.2yr., a = 0.32", motion direct. C is physical, and exhibits slow direct orbital motion. 13 26.5 +42 33 ES 2645 B is BD+43@2334. 13 26.7 -24 18 LDS 6277 C is CD-23@11076. Proper motion of C -343 -066. 13 27.4 -61 52 B 2752 A is an Algol-type system, V380 Cen. 13 27.6 +06 55 HJ 1232 Proper motion of B -057 +005. 13 27.8 +47 46 STF 1747 Proper motion of B +004 -034. 13 28.4 +13 47 STT 70 Vir. B is BD+14@2622. 13 28.8 +59 56 STF 1752 Proper motion of B -065 +028. 13 29.1 -66 04 LDS 444 B is CPD-65@2344. Proper motion of B -134 +007. 13 29.7 -23 17 HO 381 A is a Mira-type variable, R Hya. Physical pair. 13 29.8 +59 05 ES 1790 Proper motion of B +032 -007. 13 29.8 +01 06 J 2091 A is FO Vir, possibly a RR Lyrae-type variable. 13 30.3 -08 34 LDS 448 Proper motion -1093 -419. 13 30.4 -06 28 STF 1750 72 Vir. A is a spectroscopic binary. Proper motion of B +039 +002. 13 30.5 +07 29 A 1789 P = 128yr., a = 0.21", motion retrograde. 13 30.5 -23 39 HO 540 A is an Algol-type system, SS Hya. 13 30.6 -43 11 CPO 371 Nothing at this position (Heintz). 13 30.9 +24 14 H 70 AC: H V 70. C is the variable FK Com. 13 31.0 -39 24 SEE 179 P = 79yr., a = 0.16", motion retrograde. 13 31.1 -41 51 COO 155 Proper motion of B -017 -021. 13 32.0 +71 43 STF 1761 Proper motion of B +038 -016. 13 32.0 +31 08 WOR 24 P = 21.3yr., a = 0.26", motion retrograde. 13 32.0 -18 44 B 2542 73 Vir. Too close in 1951. Needs speckle. 13 32.0 -65 19 FIN 369 In rapid direct motion. 13 32.1 -22 58 HJ 4593 B is BD-22@3617, spectrum F2IV. 13 32.1 -63 03 DUN 137 Proper motion of B +001 -004. 13 32.4 +36 49 STF 1755 Spectroscopic binary. Spectral type of B: F5IV. 13 32.4 -12 40 SHJ 165 B is BD-11@3537. Proper motion of B -053 000. 13 32.8 +16 49 VYS 6 Both components are flare stars, VW Com. 13 32.9 +49 08 STF 1758 Proper motion of B -060 -016. 13 32.9 +34 54 STT 269 P = 55yr., a = 0.18", motion direct. 13 32.9 -15 22 HJ 2658 75 Vir. 13 33.2 -77 34 HJ 4590 A is a variable, S Cha. B is CPD-76@769. 13 33.3 +23 01 STF 1756 Proper motion of B -132 -004. 13 33.6 +29 44 A 1095 P = 317yr., a = 0.39", motion direct. 13 34.1 +67 46 STF 1767 Proper motion of B -174 +003. 13 34.3 -00 19 STF 1757 P = 461yr., a = 2.76", motion direct. 13 34.5 -13 26 S 650 B is BD-12@3842. Proper motion of B 000 +020. 13 34.7 -13 13 BU 932 P = 198yr., a = 0.56", motion direct. Variable? 13 34.9 +74 30 LDS 1775 Possible common proper motion with BD+75@510, about 1900" distant. 13 35.2 -35 39 HJ 4595 Proper motion of B -024 -024. 13 35.6 +10 12 HJ 228 B is BD+10@2566. Proper motion of B -024 -024. 13 36.3 +19 59 HJ 2663 Proper motion of B -037 -022. 13 36.8 -26 30 H 69 H N 69. Spectral type of B: A7IV-V. 13 37.0 +23 18 POU 3145 Proper motion of B -041 -005. 13 37.1 -16 27 RST 3845 Spectrum: F2/3III/IV. 13 37.2 +30 05 STF 1766 Proper motion of B -164 +039. 13 37.2 -61 42 I 365 P = 35yr., a = 0.46", motion retrograde. 13 37.2 -84 27 HJ 4585 B is CPD-83@531. 13 37.5 +36 18 STF 1768 25 CVn. P = 240yr., a = 1.09", motion retrograde. 13 37.7 +50 43 STF 1770 Composite spectrum; M2II-III+F3III. 13 37.7 +02 23 STF 1764 C is A of STF 1765 rej. Proper motion of B -029 -024. 13 37.7 -23 37 RST 2856 In rapid motion, but quadrant ambiguity makes inter- pretation uncertain. 13 37.9 +48 08 ES 608 At least one component is variable. 13 38.1 +39 10 STF 1769 C is BD+39@2662. Proper motion of C -224 -146. 13 38.7 +38 23 COU 1429 The KZA pairs are probably wider companions. 13 39.2 -49 00 HJ 4600 B is CD-48@8376. Proper motion of B -092 -014. 13 39.4 +35 36 AG 191 Proper motion of B -026 -022. 13 39.6 +10 45 BU 612 P = 22.3yr., a = 0.22", motion direct. 13 39.9 -53 28 RST 5376 Epsilon Cen. 13 40.7 +76 51 HJ 2682 C is BD+77@518. Proper motion of C -009 -017. 13 40.7 +59 44 HJ 2673 B is BD+60@1481. 13 40.7 +19 57 STF 1772 1 Boo. B is a metallic-line star. 13 41.4 -61 52 JSP 591 Spectrum composite: K2/3III+B8/A0V. 13 41.6 +07 36 STF 1773 Proper motion of B -003 -001. 13 41.7 -75 07 HJ 4598 Spectrum composite: A0V+G8/K0III. 13 41.8 +46 13 STF 1776 Proper motion of B -042 +013. 13 42.2 +18 07 HJ 230 Proper motion of B +006 +005. 13 43.0 -30 11 DAW 166 B variable? 13 43.1 +03 32 STF 1777 84 Vir. A is a spectroscopic binary. 13 43.3 -24 58 HJ 2671 B is CD-24@11047. Proper motion of C -039 +011. 13 43.5 -04 16 STF 1775 A is a spectroscopic binary. 13 44.0 -59 14 DUN 142 B is CPD-58@5094. Proper motion of B -038 -006. 13 44.4 +69 13 STF 1784 Proper motion of B +054 -016. 13 44.6 +51 42 KUI 64 Ross 492. 13 45.1 +18 22 STF 1782 Proper motion of B -025 +027. 13 45.1 +17 47 BUP 153 AB: Proper motion of A +427 -1810. Distance Delta declination 305" and 320". 13 45.3 -10 31 S 652 AB: B is BD-09@3768. Proper motion of B -006 -015. AC: C is BD-09@3766. 13 45.6 -15 46 HJ 2677 85 Vir. A is a spectroscopic binary and occultation triple. 13 45.8 -71 59 DUN 140 Proper motion of B -007 -003. 13 45.9 -12 26 BU 935 86 Vir. 13 46.1 +05 07 STF 1781 P = 274yr., a = 1.01", motion direct. One component is a W UMa-type eclipsing binary. 13 46.6 +28 26 KOP Bull. Harvard Coll. Obs. 1911, 1939 and JO 39, 143. 13 46.7 -36 36 POL 8 POL 2 1/2. 13 46.7 -51 26 HDO 225 A is a long-period spectroscopic binary. 13 47.0 +38 33 S 654 B is BD+39@2679. Proper motion -133 -016. 13 47.0 +06 21 LDS 3101 B is BD+07@2692. 13 47.2 -62 35 COO 157 A semiregular variable, V766 Cen. 13 47.3 +17 27 STT 270 Tau Boo. A is a Delta Scuti-type variable. 13 48.5 -43 09 HJ 4614 Proper motion of B -024 -008. 13 48.9 -35 42 HWE 94 Proper motion of B -504 -186. 13 49.0 -28 22 BU 413 A is a long-period variable, W Hya. B is CD-27@9430. Proper motion of B -130 -038. 13 49.1 +26 59 STF 1785 P = 156yr., a = 2.43", motion direct. 13 49.2 -62 06 DUN 143 Proper motion of B -011 -006. Spectral types B2(II), K2/3II/III. 13 49.3 +17 42 S 655 Proper motion of B -016 -016. 13 49.3 -40 31 DUN 146 Proper motion of B +001 +002. 13 49.6 +34 59 STF 1786 Identical with BDS 6644, HJ 852. Proper motion of B -029 -011. 13 49.6 -42 28 HDO 226 Mu Cen. A is an irregular variable. 13 50.4 +21 17 S 656 B is BD+21@2579. Proper motion of B -029 +013. BDS 6648, H VI 15 probably same star. Called a spectroscopic binary in the BSC Supplement. 13 50.5 -59 25 R 225 A variable? 13 51.4 +64 43 HJ 3342 10 Dra. A is an irregular variable, CU Dra. 13 51.4 +34 41 BU 613 C is BD+35@2495. Proper motion of C -035 +001. 13 51.5 -48 18 CPO 61 B is CD-47@8664. Proper motion of B -106 -028. 13 51.8 -33 00 H 101 H III 101. 3 Cen. 13 52.0 -47 52 HJ 4619 B is CD-47@8669. Proper motion of B -008 -013. 13 52.1 -52 49 RMK 18 Proper motion of B -057 -025. 13 53.1 +12 51 HEI 524 The Durchmusterung identification is uncertain. 13 53.2 -31 56 H 51 H N 51. 4 Cen. A is a spectroscopic binary. B is CD-31@10727. 13 53.5 -35 40 HWE 28 AB: P = 258yr., a = 1.27", motion direct. H 124 AE: H V 124. 13 53.9 -14 40 RST 3852 P = 65yr., a = 0.28", motion retrograde. 13 53.9 -19 10 HU 898 P = 317yr., 0.66", motion direct. 13 54.0 +32 09 KU 47 Proper motion of B +090 -176. 13 54.0 -47 08 HJ 4624 A is the variable V767 Cen. 13 54.0 -74 00 NZO 43 Spectrum composite: A3V+F8/G2III. 13 54.6 -50 41 BSO 9 B is CD-50@8112. 13 54.6 -66 54 DUN 145 B is CPD-66@2371. Proper motion of B -015 -016. 13 54.7 +18 24 SHJ 169 Eta Boo. A is a long-period spectroscopic binary. B is BD+19@2726. Proper motion of B -040 +017. 13 55.0 -08 04 STF 1788 AB: A premature orbit has been computed. 13 55.0 -42 35 I 401 Measures rather discordant. 13 55.9 -49 27 RST 5580 CPD-48@5937. 13 56.0 -25 32 H 59 H N 59. B is CD-24@11171. 13 56.1 -04 37 STF 1790 Proper motion of B -028 +024. 13 56.8 +14 26 STF 1791 Proper motion of B -026 -006. 13 56.9 -73 49 HJ 4621 B is CPD-73@1217. 13 57.1 -27 31 I 234 A premature orbit has been computed. 13 57.2 +11 51 HJ 233 Proper motion of B -013 -006. 13 57.2 -12 33 HJ 4637 Proper motion of B +005 -026. 13 57.3 -56 02 DUN 151 A is an irregular variable. B is CPD-55@5793. 13 57.5 -57 43 DUN 150 A is variable. 13 57.7 +52 00 A 1614 P = 1047yr., a = 2.35", motion retrograde. 13 57.9 -56 24 R 228 B is CPD-55@5797. 13 58.3 +02 13 A 2167 P = 93yr., a = 0.22", motion retrograde. 13 59.9 +25 20 BUP 156 Distances 1033.9" and 1035.6". B is BD+26@2517. Proper motion of B +002 +034. 14 00.0 -47 14 HJ 4638 C (ZZ Cen) and D (AA Cen) are variables of unknown type. 14 00.7 +24 04 BRT 3304 POU 3156 is identical, and Barton's angle is corrected by Heintz. 14 01.6 +01 33 SHJ 171 Rho Vir. A is a spectroscopic binary. B is BD+02@2760. Proper motion of B -009 -019. 14 01.8 -61 19 LPO 44 Spectral type F0? 14 02.0 +57 13 A 1097 P = 333yr., a = 0.52", motion direct. STF 1800 AB-C: C is BD+57@1479. C is optical. 14 02.0 +19 26 STF 1797 Proper motion of B -039 +016. 14 02.9 -35 11 I 1574 Measures uncertain, too close. 14 03.7 +08 29 BU 1270 P = 38.9yr., a = 0.196", motion direct. 14 03.7 +02 43 AG 192 One component is variable. 14 03.8 +56 26 LDS 2921 Proper motion of B -069 +008. 14 03.8 -60 22 VOU 31 Beta Cen. Spectroscopic and interferometric measures indicate a multiple system. 14 04.6 -35 39 I 941 Many uncertain measures. It appears nearly a revolution has been completed. 14 05.5 -36 33 DUN 154 Proper motion of B -031 -009. 14 05.6 -18 04 S 659 B is BD-17@4003. Proper motion of B +036 -043. 14 06.0 -13 04 HWE 30 Spectrum of A composite; F2, A3. Proper motion of B -028 -015. 14 06.5 +70 58 HJ 2703 Proper motion of B -035 +059. 14 06.7 -36 22 SEE 196 Theta Cen. 14 06.8 +59 46 LDS 2700 B is BD+60@1512. Proper motion of B -014 -035. 14 07.1 -63 27 HJ 4642 Spectrum composite; G0+A3. 14 07.2 -51 53 RST 681 CPD-51@6574. 14 07.5 -57 42 HJ 4645 B is CPD-57@6501. 14 07.7 -49 52 SLR 19 P = 233yr., a = 1.07", motion direct. 14 07.7 -53 41 DUN 155 B is CPD-53@5880. Proper motion of B -050 -026. 14 07.7 -57 38 R 238 First distance? B is CPD-57@6504. 14 08.2 -50 19 CPO 382 CPD-49@6690. 14 08.3 +49 27 H 112 H VI 112. 13 Boo. A is the variable CF Boo. 14 08.3 +21 12 STF 1804 Proper motion of B -021 -040. 14 08.6 +06 02 HJ 2701 Proper motion of B -036 -027. 14 08.7 +33 41 HU 742 A premature orbit has been computed. 14 08.8 +77 33 BAG 4 UMi. A spectroscopic binary, P = 605.8d, now resolved. 14 08.8 +48 30 STF 1806 Proper motion of B -034 +046. 14 09.0 -10 20 CHR 40 96 Vir. 14 09.5 +35 49 HJ 540 Proper motion of B -049 +027. 14 09.6 -51 30 HJ 4651 A is a spectroscopic binary and may be variable. B is CD-50@8297. 14 11.0 +50 15 STF 1814 Proper motion of B -179 +145. 14 11.2 -35 52 COO 287 Proper motion of B -021 +023. 14 11.5 +73 00 H 178 H V. 14 12.2 +44 11 STT 278 P = 243yr., a = 0.36", motion retrograde. 14 12.3 +02 25 HJ 3343 A is the Alpha CVn-type variable CU Vir. 14 12.4 +03 52 A 1797 Too close 1956. 14 12.8 +11 04 A 1099 Round 1951-1962. 14 13.1 +55 20 STF 1820 A premature orbit has been computed. 14 13.4 +05 24 STF 1813 Proper motion of B +028 +023. 14 13.5 +51 47 STF 1821 Kappa Boo. A is a Delta Scuti-type system. B is a long- period spectroscopic binary with P = 1791.2d. Proper motion of B +103 -012. 14 13.5 +12 34 BU 224 P = 252yr., a = 0.60", motion retrograde. 14 13.8 +30 59 COU 606 P = 24.2yr., a = 0.16", motion retrograde. 14 13.9 -58 03 JSP 618 CD-57@5471. 14 14.1 +12 58 CHR 41 14 Boo. A spectroscopic binary with P = 726.6d. 14 14.1 -50 29 BRT 825 CPD-49@6779. 14 14.2 +59 15 STF 1827 Proper motion of B -072 +012. 14 14.2 -08 31 BU 939 P = 600yr., a = 0.80", motion retrograde. 14 14.2 -51 11 CPO 383 CPD-50@6728. 14 14.5 -29 14 HJ 4664 Proper motion of B -048 -019. 14 14.8 +10 06 KUI 66 15 Boo. 14 15.0 -57 05 HDO 228 A is the variable V795 Cen. 14 15.2 +22 16 LDS 954 Proper motion of B +090 -149. 14 15.3 +03 08 STF 1819 P = 220yr., a = 1.12", motion retrograde. 14 15.7 +56 40 STF 1830 AB: Proper motion of B -023 +028. 14 15.8 +10 18 A 1101 Ambiguous case. P = 34 or 72yr., a = 0.21 or 0.32", motion retrograde. STF 1823 AB-C: C is physical. 14 16.0 +56 41 STF 1831 C is D of STF 1830. 14 16.0 -07 04 HU 138 P = 151yr., a = 0.46", motion direct. 14 16.2 +51 22 STF 26 Iota Boo. A is a spectroscopic binary and a Delta Scuti-type variable, P = 0.027d. B is BD+52@1785. Proper motion of B -142 +079. 14 16.2 +32 35 HZG B is BD+33@2434. 14 16.4 -52 25 RST 692 Proper motion of B -068 -015. 14 16.5 +33 34 HU 1266 P = 39yr., a = 0.16", motion direct. Possibly an ambi- guous case, although only one solution has been tested. 14 16.5 +20 07 STF 1825 Proper motion of B -155 -110. 14 16.5 +01 45 H 1 H N 1. 14 16.5 -57 18 BSO 10 B is CPD-56@6216. 14 16.6 -59 55 I 366 A is the Mira-type variable R Cen. 14 17.1 +01 03 HJ 1250 Proper motion of B +049 -103. 14 17.1 -48 10 HJ 4666 B is CD-47@9026. 14 17.5 +17 22 A 2067 Round 1952-1957, 1968-1975. 14 17.8 +48 45 HJ 2710 C is BD+49@2286. Proper motion of C +011 +009. 14 17.9 +69 14 A 1102 P = 225yr., a = 0.35", motion retrograde. 14 19.0 +24 06 HJ 2708 Proper motion of B -002 +024. 14 19.2 +42 23 AG 193 Proper motion of B -110 +006. 14 19.3 +13 00 ENG 51 18 Boo. 14 19.5 -68 38 I 325 B is CPD-68@2106. 14 19.9 +67 47 STF 1840 Proper motion of B -021 +009. 14 20.3 +48 30 STF 1834 P = 321yr., a = 0.90", motion direct. 14 20.6 -37 53 SEE 204 Psi Cen. 14 21.5 +53 54 STF 1839 Proper motion of B +001 -004. 14 21.8 +03 55 BAL 2861 A is the Mira-type variable AO Vir. 14 22.5 -25 18 RST 5534 Measures discordent by 90@ in 1951. 14 22.6 -58 28 DUN 159 A is a spectroscopic binary. 14 23.4 +08 27 STF 1835 Mt. Wilson spectral types A1n and F1s. A is physical. BU 1111 BC: P = 39.5yr., a = 0.23", motion direct. Spectra of BC, F0V+F2V. 14 24.1 +11 15 STF 1838 BDS 6833, H III 20 probably same star. Proper motion of B +048 +004. 14 24.3 -38 38 RST 1785 P = 83yr., a = 0.22", motion direct. 14 24.6 +47 50 STF 1843 Proper motion of B -050 -034. 14 25.2 +51 51 STT Theta Boo. A is a Delta Scuti-type variable. 14 25.7 +23 38 BU 1442 AB: Proper motion +786 -1118. 14 25.8 +22 17 HJ 2721 B is BD+22@2700. 14 25.9 -21 08 BHA 17 CPD-20@5922. 14 25.9 -37 13 RST 2904 Spectrum: A8/9II/III. 14 26.1 -45 13 DUN 160 Tau (1) Lup. Variable. B is CD-44@9321. 14 26.2 -45 23 I 402 Tau (2) Lup. P = 26.2yr., a = 0.12", motion direct. 14 26.5 -50 34 CPO 388 CPD-50@6917. 14 26.6 +02 08 HJ 1254 Proper motion of B -121 +106. 14 26.7 +16 25 A 2069 P = 42yr., a = 0.20", motion retrograde. 14 27.5 +75 42 HJ 2733 5 UMi. 14 27.9 +21 23 HO 543 Proper motion of B +035 -103. 14 28.2 -02 14 STF 1846 Phi Vir. B is a spectroscopic binary. 14 28.2 -29 29 FIN 306 52 Hya. 14 28.6 +28 17 STF 1850 B is BD+28@2331, and is a spectroscopic binary. Proper motion of B +014 +002. 14 28.7 -10 12 STF 1847 B is BD-09@3946. Proper motion of B -060 +017. A measure of A and BD-09@3950: 1907.26, Delta (delta) 190.80". 14 29.1 +69 17 MLR 170 The scattered measures and quadrant ambiguity make determination of the direction of motion impossible. 14 29.3 -01 43 FIL 28 Proper motion of B -048 +006. 14 29.5 +36 12 HU 1268 A premature orbit has been computed. 14 30.3 -49 31 HDO 232 A is a spectroscopic binary, spectrum composite; A1V+B. 14 30.7 +83 08 LDS 1800 Proper motion of B +116 -067. 14 30.8 +04 46 BU 1443 See BDS 6932. Burnham could not find star measured by Madler. No star in or near Madler place. B is BD+05@2885. 14 30.8 -08 39 BUP 158 Proper motion -1272 -236. 14 30.8 -50 29 LDS 490 B is CD-49@8796. 14 31.0 -05 48 RST 4529 Ambiguous case. P = 25 or 45yr., a = 0.27 or 0.32", motion direct. 14 31.4 +34 30 HU 904 Van Biesbroeck and Fox identify this pair as BD+35@2575, but Hussey says it is 5.59s following and 4' 46.4" north of that star. 14 31.7 +01 50 AG 195 Heintz believes HJ 5485 is identical; there is no pair in the place formerly assigned to Herschel's pair. 14 31.8 +30 22 HJ 2728 Rho Boo. Proper motion of B +013 +003. 14 32.1 +38 18 BLM Gamma Boo. A is a Delta Scuti-type system. 14 32.3 +80 20 STT 130 B is BD+80@444. Proper motion of B -022 +028. 14 32.3 +26 41 A 570 P = 29.9yr., a = 0.20", motion retrograde. 14 32.3 +17 18 STF 3086 Proper motion of B -004 -001. 14 32.4 +31 38 STF 1855 Proper motion of B +031 -045. 14 32.5 +34 42 HJ 554 Proper motion of B +037 -029. 14 32.7 -12 46 GLP 3 B is BD-12@4080. 14 32.9 +41 26 HJ 1255 B is BD+42@2510. 14 34.3 +24 24 STT 129 B is BD+25@2797. Proper motion of B +004 -007. 14 34.5 +05 40 J 1122 A measure in 1952: 279.2@, 1.4". The 1957 measure may be inaccurate. 14 34.5 -63 17 HJ 4683 Spectrum of B: A8/F0. Proper motion of B -014 -022. 14 34.7 +29 45 STT Sigma Boo. Possibly variable. 14 35.1 -61 01 B 2338 A is the Cepheid TX Cen. 14 35.8 +06 20 MAD 6 Not found by Burnham. 14 36.3 -46 15 HDO 236 A is variable. 14 36.7 +12 10 STF 1861 Proper motion of B -037 +003. 14 36.9 +48 13 A 347 P = 151yr., a = 0.49", motion retrograde. 14 37.5 -29 41 WNO B is CD-29@11196. Proper motion of B -102 -026. 14 37.8 +14 54 STF 1862 Proper motion of B -026 -014. 14 38.0 -54 31 DUN 163 B is CPD-53@6038. Proper motion of B -017 -013. 14 39.5 -68 12 MLO 58 The primary is slightly variable. 14 39.6 -60 50 RHD 1 Alpha Cen. P= 79.9yr, a = 17.52", motion direct. Proper motion -3642 +699. The distant companion, Proxima Centauri, distance 9000" was discovered by Innes. It is the flare star V645 Cen. 14 40.3 +48 43 STT 284 Proper motion of B -084 -111. 14 40.3 -45 48 SEE 209 The primary is slightly variable. 14 40.4 +21 59 MCA 40 P = 9.27yr., a = 0.071", motion retrograde. 14 40.7 +16 25 STF 1864 Pi (1) Boo. Proper motion of B -018 +006, spectrum A6V. Both components are spectroscopic binaries. 14 41.0 +57 57 STF 1872 Proper motion of B +145 -163. 14 41.1 +13 44 STF 1865 Zeta Boo. P = 123yr., a = 0.60", motion retrograde. H 104 H IV 104. 14 41.9 -47 23 HDO 238 Alpha Lup. Variable. 14 42.1 +61 16 STF 1878 A is the Delta Scuti-type variable DL Dra. 14 42.2 +49 07 STF 1874 Proper motion of B -023 +015. 14 42.5 -64 59 DUN 166 Alpha Cir. Probably variable. 14 42.6 +19 29 HU 575 P = 52yr., a = 0.63", motion retrograde. BD+20@3009 has common proper motion, and is component C (LDS 968). 14 42.7 -05 58 STF 1869 B is BD-05@3935. Proper motion of B -058 +017. 14 43.0 +13 10 KU 48 Proper motion of B -013 +050. 14 43.5 -62 58 B 1759 C is variable. 14 44.3 -27 01 B 276 ADS 9359a. 14 44.5 +33 45 HJ 556 Proper motion of B -027 +006. 14 44.8 +07 42 STF 1873 Proper motion of B -001 -009. 14 45.0 +27 04 STF 1877 Epsilon Boo. B is a spectroscopic binary. 14 45.2 -55 36 DUN 169 The primary is BU Cir, a Beta CMa-type variable. B is CPD-55 6152. 14 45.3 -36 09 I 528 Too close, measures uncertain. 14 45.5 +42 23 STT 285 P = 88.4yr., a = 0.32", motion retrograde. There is a faint common proper motion companion (Mag. 12.5, 50"). 14 46.0 -15 28 HLD 20 5 Lib. 14 46.0 -25 27 H 97 H III 97. 54 Hya. Proper motion of B -116 -121. 14 46.2 -21 11 FIN 309 17 Lib. P = 26yr., a = 0.30", motion direct. 14 46.3 +09 39 STF 1879 P = 226yr., a = 0.99", motion retrograde. 14 46.4 -78 47 HJ 4689 B is CPD-78@889. 14 47.1 -73 29 HJ 4693 B is CPD-72@1571. 14 47.7 +24 06 HO 263 Suspected double by HO, but unconfirmed by many other observers; duplicity still in doubt. 14 47.9 -33 25 HJ 2744 Proper motion of B +003 +003. 14 48.2 +09 29 L Single in 1952, 1958, 1959. 14 48.9 +05 57 STF 1883 P = 228yr., a = 0.84", motion retrograde. 14 49.2 +10 13 A 2983 Ambiguous case. P = 9.9 or 19.8yr., a = 0.17 or 0.16", motion direct. 14 49.2 -59 24 FIN 298 Motion direct. 14 49.3 -14 09 BU 106 Mu Lib. 14 49.3 -24 15 H 117 H VI 117. 14 49.5 +51 22 STF 1889 Both components are spectroscopic binaries. Proper motion of B -003 +012. 14 49.7 +48 43 STF 1890 39 Boo. B is a spectroscopic binary. Proper motion of B -078 +091. Spectral types F6V+F5V. 14 49.7 -43 00 CPO 402 B is CD-42@9693. 14 50.4 -66 25 FIN 426 Spectrum: G8/K1(IV)+A/F. 14 50.5 -70 32 HJ 4697 B is CPD-70@1824. Proper motion of B -090 -007. 14 50.6 -00 01 STF 1885 Proper motion of B +018 +019. 14 50.7 +74 09 BUP 159 Beta UMi. 14 50.9 -16 03 SHJ 186 Alpha (2) Lib. B is BD-15@3965. Proper motion of B -088 -056. A is a spectroscopic binary. 14 51.0 +09 43 STF 1886 BDS 7052; MAD same star. 14 51.1 -37 06 I 529 A premature orbit has been computed. 14 51.1 -61 53 JSP 640 CD-61@4558 14 51.3 -17 00 HU 1270 AB is fainter than C (van den Bos). Proper motion of B -001 -002. 14 51.4 +44 36 HJ 2752 Proper motion of B +004 +040. 14 51.4 +19 06 STF 1888 Xi Boo. P = 151.5yr., a = 4.90", motion retrograde. 14 51.5 +44 56 STT 287 P = 400yr., a = 0.93", motion direct. 14 51.6 -43 35 FIN 319 Omicron Lup. 14 51.7 -30 53 H 48 H N 48. B is CD-30@11767. Proper motion of B -063 -068. 14 52.3 -44 55 DON 689 CPD-44@7016. 14 52.6 -11 51 LDS 511 B is BD-11@3820. 14 52.6 -42 05 HJ 4710 Proper motion of B -031 -053. 14 53.3 -52 20 CPO 403 CPD-51@8545. 14 53.4 +15 42 STT 288 P = 210yr., a = 0.96", motion retrograde. 14 53.4 -45 51 DUN 171 Proper motion of B -008 +005. 14 53.5 -46 37 B 2774 A (S Lup) and B (X Lup) are both variable. 14 54.0 +23 35 REU 2 P = 34yr., a = 0.69", motion retrograde. 14 54.0 -63 33 RST 730 RST 730a. 14 54.2 -66 25 HJ 4707 P = 288yr., a = 1.39", motion retrograde. 14 54.5 +16 06 FRT 1 The companion is of spectral type dM8.5.e. The measure was made in the infrared. 14 54.6 -33 18 BU 347 CPD-32@3746. 14 54.7 +50 38 AG 196 Proper motion of B -030 +018. 14 55.4 +00 10 A 2171 Single 1946, 1951. 14 55.4 -55 26 HJ 4712 Proper motion of B -062 -040. 14 55.8 +39 39 A 1627 P = 101yr., a = 0.232", motion direct. 14 56.5 -34 38 I 227 AB: P = 40yr., a = 0.26", motion retrograde. B 2778 AB-C: C is probably physical. SEE 215 AB-D: CPD-34@6262. 14 56.5 -47 53 HJ 4715 The primary is a spectroscopic binary. 14 56.6 -14 06 HJ 561 B is BD-13@4022. Proper motion of B +007 +027. 14 56.7 -62 47 FIN 372 Theta Cir. One component is variable. 14 56.8 +74 54 S 666 8 UMi. B is BD+75@549. 14 57.0 +17 58 KU 106 Proper motion of B +020 -007. 14 57.4 +85 29 BU 353 Proper motion of B -102 +072. 14 57.5 +40 10 STF 1895 Proper motion of B +010 -005. 14 57.5 -21 25 H 28 AB: H N 28. B is BD-20@4123. Proper motion of B +1000 -1662. B is a spectroscopic binary, P = 308d. 14 57.6 -00 10 H 51 H V 51. 14 57.8 +08 16 HJ 2756 Proper motion of B -037 -021. 14 58.0 -63 33 HJ 4714 B is CPD-63@3460, spectrum B8/A0III/IV. 14 58.5 -47 26 CPO 62 B is CD-46@9704. Proper motion of B -036 -028. 14 58.7 -27 39 BU 239 59 Hya. A premature orbit has been computed. Alternative spectra:; A4V+A6V. 14 58.9 -11 09 STF 1894 18 Lib. Proper motion of B +044 +125. 14 59.2 -42 06 I 1260 Kappa Cen. A spectroscopic binary and variable star. 14 59.6 +53 52 SHJ 191 B is BD+54@1724. Proper motion of B +021 -004. 15 00.2 -58 56 HJ 4719 B is CPD-58@5778. Proper motion of B -024 000. 15 00.6 +47 17 STT 291 A is the Alpha CVn-type variable BX Boo. Proper motion of B -008 +015. 15 01.0 +31 23 STF 1901 BU gives Delta(delta) from BD+31@2685. 1871.3, 112.3". 1907.2, 109.9". Proper motion of B 000 -004. SEI 538. 15 01.0 -08 31 J 1586 Delta Lib. A is an Algol-type system. 15 01.6 -42 23 I 1263 Spectrum K0/2III+A3/5 15 01.8 +05 38 HJ 2760 Proper motion of B -006 -010. 15 01.8 -36 56 HJ 4724 Proper motion of B -042 +019. 15 01.9 +15 47 STF 1902 Proper motion of B -009 -057. 15 02.4 -47 23 BRT 843 CPD-46@7153. 15 02.5 +47 45 H 53 This star was measured for H VI 53, which could not be identified. 15 03.2 +07 40 HJ 1267 Proper motion of B -071 -029. 15 03.5 -40 35 I 1262 P = 134yr., a = 0.29", motion direct. 15 03.8 +47 39 STF 1909 44 Boo. P = 225yr., a = 3.77", motion direct in a highly-inclined orbit. Proper motion of B -388 +034. B is a W UMa-type eclipsing binary. 15 04.1 +05 30 STF 1904 Proper motion of B 000 -031. 15 04.2 -15 30 RST 3906 P = 41yr., a = 0.24", motion retrograde. 15 04.2 -51 20 B 1258 Spectrum A5/7III/IV 15 04.3 +29 05 BU 1445 This may be HJ 564 (Burnham). 15 04.4 -49 45 HJ 4726 Spectrum A3/5II/III 15 04.5 -17 54 S 665 B is BD-17@4247. Proper motion of B -023 -003. Spectrum of A: K2IIICNIb/II, of B: K0III. 15 05.1 -47 03 HJ 4728 Pi Lup. Both components are spectroscopic binaries. 15 05.3 -19 36 RST 3907 Spectrum Fm Delta Del. 15 05.9 +03 50 BAL 2867 Proper motion of B -009 +021. 15 06.8 -16 29 BUP 160 22 Lib. 15 07.1 -02 17 A 689 P = 66yr., a = 0.31", motion retrograde. 15 07.3 +24 52 ENG 52 45 Boo. 15 07.3 +18 27 A 2385 P = 8yr., a = 0.10", motion retrograde. 15 07.5 +09 14 STF 1910 Proper motion of B -182 +024. 15 07.8 +63 07 STF 1918 A is a spectroscopic binary, P = 2.45d. 15 07.8 -73 50 B 2028 Spectrum of B: A/F. 15 08.0 -48 27 BRT 848 CPD-47@6912. 15 08.0 -48 45 CPO 414 CPD-48@7127. Heintz was unable to find this pair. 15 08.7 -51 40 BRT 849 CPD-51@7573. 15 08.8 -45 17 SEE 219 Lambda Lup. P = 65yr., a = 0.35", motion direct. There is probably a spectroscopic subsystem. 15 09.1 +05 12 STF 1912 Proper motion of B -040 -005. 15 09.3 +72 27 STF 1928 Proper motion of B -049 +015. 15 09.6 -68 43 DON 714 T TrA. Uncertainly variable. 15 10.3 -16 16 BUP 161 A : Proper motion -1016 -3571. BUP 161 AC: Proper motion of C -1033 -3526. 15 10.7 -43 44 CPO 415 B is CPD-43@9678, spectrum K0IV-V. Proper motion of B +015 -111. 15 10.8 +46 51 STF 1920 Proper motion of B -078 +030. 15 11.2 -59 24 HRG 105 B is CPD-58@5840, spectrum A5V. 15 11.5 -54 43 RST 2942 Composite-like spectrum: G8/K0III+F/G. 15 11.6 -32 08 HJ 2765 B is CD-31@11773. 15 11.7 -05 29 STF 1914 B is BD-04@3827. Proper motion of B -038 -018. 15 11.8 +61 51 STF 1927 A and B are both W UMa systems, BV and BW Dra., periods 0.29 and 0.35d. Spectra F9V, F8V and G3V and G0V. Proper motion of B -154 +088. 15 11.9 -32 50 HJ 4743 Proper motion of B -004 -003. 15 11.9 -48 44 DUN 177 Kappa (1) Lup. B is CD-48@9705, Kappa (2) Lup. Proper motion of B -097 -042. 15 12.0 +38 40 STF 1921 B is BD+39@2844. Proper motion of B +023 -009. 15 12.1 +34 19 POP 209 Co-discovered by Olevic. 15 12.1 +18 59 COU 189 The variable FL Ser. 15 12.2 -19 48 B 2351 Iota (1) Lib. P = 23.4yr., a = 0.12", motion retro- grade. There is evidence for a spectroscopic subsystem, and BC is physical, so the system is probably quin- tuple. Alternate spectrum of Aa: ApSi. H 44 Aa-B: H VI 44. 15 12.3 -52 06 DUN 176 Zeta Lup. B is CD-51@8827. Proper motion of B -099 -073. 15 12.7 +60 08 HU 1159 P = 144yr., a = 0.21", motion direct. 15 12.7 +19 17 STF 1919 Proper motion of B -594 +276. 15 12.7 -47 58 CPO 64 B is CD-47@9781. Proper motion of B -108 -037. 15 12.8 +27 56 H 125 H V 125. B is BD+28@2411. Proper motion of B +012 -124. 15 13.6 +34 53 HO 60 P = 189yr., a = 0.28", motion retrograde. 15 13.8 -01 21 A 691 Close, rapidly moving, quadrant uncertain. Proper motion of A -1266 -504. 15 14.0 -41 28 HJ 4748 B is CD-40@9410. 15 14.1 +31 47 STT 292 B is BD+32@2562. Proper motion of B -022 +010. 15 14.1 +01 43 ABT 11 ABT calls this BDS 7169, HJ 1269. 15 14.3 -36 13 GLP 10 B is CD-35@10137. 15 14.3 -42 42 B 1273 CPD-42@6958. 15 14.5 -18 26 SHJ 195 B is BD-17@4284. Proper motion of B -109 -020. 15 14.5 -43 23 DUN 179 Proper motion of B -037 -043. 15 14.9 +50 48 ES 775 Proper motion of B +040 +004. 15 15.3 -44 09 HDO 244 Proper motion of B -017 -027. 15 15.4 -55 44 HJ 4747 B is CPD-55@6450. 15 15.5 +33 19 STF 27 Delta Boo. A is a spectroscopic binary. B is BD+33@2562. Proper motion of B +088 -103. 15 15.8 +50 56 STT 137 B is BD+51@1992. Proper motion of B -023 +015. 15 15.8 -37 09 COO 271 Proper motion of B -029 -017. 15 16.0 -04 54 STF 3091 P = 156yr., a = 0.37", motion retrograde in a highly- inclined orbit. 15 16.9 -60 57 HDO 245 Delta Cir. A variable and spectroscopic binary. 15 17.1 -59 48 I 1074 I 1074 1/2. 15 17.3 +71 13 H 86 H V 86. 15 17.4 +43 48 STF 1934 Proper motion of B -075 +007. 15 17.9 -23 23 I 1268 CD-22@10926. 15 17.9 -74 35 I 330 Composite-like spectrum: G8/K0(III)+A. 15 18.3 +26 50 STF 1932 P = 203yr., a = 1.22", motion direct. The recently found sub-system must have a short period. There is also evidence of light-variability in the system. 15 18.5 -47 53 HJ 4753 Mu Lup. 15 18.7 +10 26 STF 1931 Proper motion of B -071 +012. C is slightly variable. 15 19.3 +01 46 STF 1930 5 Ser. AB: Mt. Wilson spectral types F5s, M0. AD: See BDS and ADS for rectangular measures. 15 20.1 +29 37 ENG 53 Omicron CrB. Proper motion of B +022 -039. 15 20.2 +30 42 STF 1935 Proper motion of B +006 -014. 15 20.6 +15 23 HU 1160 A premature orbit has been computed. 15 21.0 +00 43 BU 32 6 Ser. Possibly variable. 15 21.0 -15 33 BU 1447 Omicron Lib. 15 21.1 +27 02 STF 1936 Proper motion of B -003 +008. 15 21.8 -02 01 STF 3092 Proper motion of B +031 -063. 15 21.8 -36 16 SEE 229 Phi (1) Lup. 15 22.0 -15 05 H 132 H V 132. This is either BDS 7219 or 7223. 15 22.2 +45 08 ES 2649 B is BD+45@2281. 15 22.6 -47 55 SLR 20 Motion retrograde. 15 22.7 -01 32 STF 3093 Proper motion of B -075 +029. 15 22.7 -44 41 COP 2 Epsilon Lup. A is a spectroscopic binary. 15 23.0 +11 22 AG 347 Proper motion of B -013 -016. 15 23.2 +30 17 STF 1937 Eta CrB. AB: P = 41.6yr., a = 0.91", motion direct. 15 23.3 +36 19 A 1367 AB-C: Identification doubtful. 15 23.4 -59 19 HJ 4757 Gamma Cir. A premature orbit has been computed. 15 24.1 -33 02 HJ 4765 A is probably a Mira-type variable, GN Lup. 15 24.5 +37 23 CHR 181 Mu (1) Boo. A is a long-period spectroscopic binary. STF 1938 BC: Mu (2) Boo. P = 246yr., a = 1.40", motion retrograde. 15 24.5 -17 00 BHA 57 Proper motion of B +021 -022. 15 24.8 -39 43 RST 1839 Upsilon Lup. 15 24.9 +58 58 BUP 162 Iota Dra. B is BD+59@1655. 15 25.2 -46 59 RST 767 P = 187yr., a = 0.41", motion direct. 15 25.2 -47 13 RST 766 CPD-46@7410. 15 26.1 +21 28 STF 1942 Proper motion of B +003 +018. 15 26.2 -28 19 RST 769 P = 142yr., a = 0.42", motion retrograde. 15 26.3 -42 52 DUN 184 B is CD-42@10392. Proper motion of B -010 -012. 15 26.5 +43 51 BU 1449 B is BD+44@2468. 15 26.6 +54 54 STF 1948 Proper motion of B -012 +012. 15 26.6 -17 06 HU 309 Spectrum: F3/5III/IV. 15 26.7 -52 54 B 2354 Not found by Heintz. 15 26.9 +46 10 KU 50 The pair L 13 formerly listed at 15280+4612 is identical (Heintz). 15 27.3 +17 38 A 2074 P = 59yr., a = 0.21", motion direct. 15 27.3 +09 42 A 1120 P = 50yr., a = 0.19", motion direct. 15 27.6 +05 22 STF 1943 Proper motion of B -030 -005. 15 27.7 +42 53 KU 108 Proper motion of B -049 -260. 15 27.8 +29 06 JEF 1 Beta CrB. A spectroscopic binary resolved visually, and a variable of Alpha CVn-type. P = 10.3yr., a = 0.205", motion retrograde. 15 28.0 +14 42 STF 1945 Proper motion of B -017 +110. 15 28.2 +02 51 A 2175 P = 160yr., a = 0.24", motion direct. 15 28.2 -09 21 SHJ 202 BDS 7220, H V 27 same star. The primary is a spectro- scopic binary of very high eccentricity, P = 889.6d. C is BD-08@3984, and is optical. A 15.35mag. star at 20' shares common proper motion. 15 28.2 -37 22 RST 3920 The primary is the variable GO Lupi. 15 28.4 -39 03 RST 1841 Proper motion of B -011 +010. 15 28.8 -34 20 SEE 235 Spectrum: G8/K0III/IV. 15 29.2 +80 27 STF 1972 A is a spectroscopic binary. Composite spectrum: G0IV-V+G8IV-V. B is BD+80@481, and is also a spectro- scopic binary. Proper motion of B -219 +104. 15 29.4 +67 12 STF 1958 B is BD+67@899. 15 29.9 +05 52 GAU 14 Observed for HJ 2782, but evidently a different pair. 15 30.3 +15 43 HJ 254 Proper motion of B -007 +016. 15 30.6 +13 03 STF 1949 Proper motion of B -001 -025. 15 30.7 +38 10 HU 1163 P = 234yr., a = 0.29", motion direct. 15 31.2 -18 52 HO 393 Burnham connects A with BD+18@4083. 15 31.3 -12 59 BU 33 AE: Fox in 1926 and van den Bos in 1959 reverse the quadrant. 15 31.5 -73 23 HJ 4764 Kappa (1) Aps. A is variable. 15 31.7 -20 10 S 672 A is a spectroscopic binary. 15 31.8 +40 54 A 1634 Nu (2) Boo. An example of adequate resolution provided only by speckle: P = 8.48yr., a = 0.060", motion retrograde. 15 32.5 +81 03 STF 1980 Proper motion of B -001 -010. 15 32.5 +08 35 STT 140 B is BD+09@3061. Proper motion of B -019 +011. 15 32.5 -52 52 HJ 4778 B is CPD-52@8474. 15 32.5 -77 31 HJ 4760 Spectral types: B7(III)+B/A. B is CPD-77@1124. 15 32.8 +19 45 HU 577 P = 112yr., a = 0.28", motion direct. 15 32.9 +31 22 COU 610 Theta CrB. Variable. 15 32.9 +05 31 STF 1953 Proper motion of B -030 +002. 15 33.1 -58 12 DUN 186 B is CPD-57@7083. Proper motion of B -056 -062. 15 33.2 -24 29 LAL 123 A-BC: A is physical. SEE 238 BC: P = 60.4yr., a = 0.24", motion direct. 15 33.6 -47 32 DUN 187 CPD. B is CPD-47@7206. 15 33.9 +63 54 STT 299 A is the Algol-type system TW Dra. 15 33.9 +26 43 STF 1955 Proper motion of B +034 -030. 15 34.6 +44 54 HJ 2788 B is BD+45@2304. 15 34.6 +43 31 STF 1961 Proper motion of B -041 +076. 15 34.8 +10 32 STF 1954 Delta Ser. A premature orbit has been computed. The primary is a Delta Scuti-type variable. 15 35.1 -41 10 HJ 4786 Gamma Lup. P = 190yr., a = 0.66", motion retrograde in a highly-inclined orbit. 15 35.4 +17 43 LDS 977 Ross 513. 15 35.5 -14 47 WRH 20 Aa: Uncertain duplicity. GOL Aa-B: Gamma Lib. 15 35.7 -80 12 HJ 4759 B is CPD-79@845. 15 35.9 -44 57 HJ 4788 A is a spectroscopic binary. 15 36.0 +39 48 STT 298 AB: P = 55.6yr., a = 0.80", motion direct. AB-C: C is physical. 15 36.0 -49 30 RST 780 A is the Mira-type variable R Nor. 15 36.0 -50 51 B 2359 CPD-50@8274. 15 36.6 +09 15 STF 1960 Proper motion of B -065 +018. 15 36.7 -66 19 DUN 188 Epsilon TrA. B is CPD-65@3101. Proper motion of B 000 -014. 15 37.0 +64 26 HU 1168 P = 89yr., a = 0.39", motion retrograde. 15 37.0 -00 41 HJ 1276 Proper motion of B -024 -005. 15 37.0 -28 08 I 1271 Upsilon Lib. 15 37.2 -23 39 SEE 241 B 296. Misidentified by See. 15 37.9 +30 06 STF 1963 Mt. Wilson spectral types F5s and G1. 15 38.1 -42 34 HDO 250 Omega Lup. Variable velocity. 15 38.7 -08 47 STF 1962 A is a spectroscopic binary. B is BD-08@4031. Proper motion of B +026 -030. 15 38.9 +57 28 STT 141 AB: B is BD+57@1599. Proper motion of B -017 +026. 15 39.0 +25 45 COU 612 P = 33yr., a = 0.18", motion retrograde. 15 39.4 +36 38 STF 1965 Zeta (2) CrB. A is a spectroscopic binary. B is Zeta (1) CrB. Proper motion of B -017 -023. 15 39.6 +79 59 STF 1989 Pi UMa. P = 188yr., a = 0.44", motion retrograde. 15 40.2 +12 03 STT 300 A is a spectroscopic binary, spectrum G7.5IIIaCN- Fe0.5. Proper motion of B -009 +001. 15 40.4 -73 27 HDO 249 Kappa (2) Aps. 15 41.3 +59 59 STF 1969 P = 325yr., a = 0.82", motion direct. 15 41.4 -29 10 RST 1855 CPD-28@5170. 15 41.6 +19 40 HU 580 Iota Ser. Ambiguous case, P = 11 or 22yr., a = 0.12 or 0.22", motion direct, highly-inclined. Spectroscopic evidence shows a third star present in the system. 15 41.8 -42 25 CPO 440 B is CD-42@10665. 15 41.9 -19 41 ENG 54 Kappa Lib. A has variable velocity. B is BD-19@4187. 15 41.9 -30 09 ARG 28 B is CD-29@11878. Proper motion of B -033 -034. 15 42.0 +00 27 A 2176 P = 56yr., a = 0.19", motion direct. One component is a short-period spectroscopic binary. 15 42.0 -11 08 STF 1966 Proper motion of B +061 -022. 15 42.1 -67 31 DON 1114 CD-67@1794. 15 42.7 +26 18 STF 1967 Gamma CrB. P = 93yr., a = 0.73", motion retrograde, highly-inclined orbit. A is a Delta Scuti-type variable. 15 42.7 -34 43 ISO 1 Psi (2) Lup. The pair is also a double-lined spectro- scopic binary, P = 12.26d. 15 43.0 +26 17 LDS 4588 Proper motion of B +107 -049. 15 43.0 -58 07 DUN 190 Spectrum of B: B8/A0(III). 15 43.2 +13 40 BU 619 One component is a spectroscopic binary. 15 43.5 -51 51 HJ 4794 B is CD-51@9412. B is the Algol-type system HH Nor. 15 44.0 +02 31 A 2230 Psi Ser. AC: C is BD+02@2988. CE: E is BD+02@2987. 15 44.3 +06 26 HJ 1277 Alpha Ser. Variable? 15 44.8 +35 34 PRT 5 Proper motion of B +002 -044. 15 44.9 +59 26 STF 1976 Proper motion of B -009 000. 15 45.2 -38 19 LDS 539 Spectrum of B sdF5. 15 45.3 -58 41 FIN 234 Spectrum composite: G5/8III+A3/7. 15 45.4 -01 23 STF 1968 Proper motion of B -050 -017. 15 45.7 +50 40 HU 657 P = 381yr., a = 0.57", motion retrograde. 15 46.1 -01 48 ISO 2 25 Ser. A spectroscopic binary, P = 38.9d. 15 46.2 +15 25 STF 1970 Beta Ser. Proper motion of B -069 -058. 15 46.4 +36 27 STF 1973 B is BD+36@2644. Proper motion of B -094 +052. 15 46.7 -34 41 B 847 Measures uncertain; too close. 15 47.6 +83 16 STF 2002 B is BD+83@455. Proper motion of B +001 -018. 15 47.6 +55 23 BU 946 A is a spectroscopic binary. 15 49.3 +60 32 HU 912 P = 109yr., a = 0.32", motion direct. 15 49.5 +25 28 STF 1977 Griffen and Duquennoy (Observatory 113, 128; 1993) report that the primary is composed of a SpB1 plus a more distant companion. Thus the system is quadruple. Proper motion of B -047 +008. 15 50.7 +22 29 STF 1979 Proper motion of B +003 +022. 15 50.9 +14 41 STF 1978 Proper motion of B -015 +015. 15 51.1 -55 03 DUN 193 A is a spectroscopic binary. Spectrum of B may be K. Proper motion of B -029 -053. 15 51.2 +35 39 BUP 163 Kappa CrB. 15 51.3 -03 05 CHR 51 36 Ser. 15 52.0 +52 34 AG 199 B is BD+52@1912. Proper motion of B +022 +020. 15 52.2 -29 53 HO 397 A variable? 15 53.1 +34 45 LDS 6309 Ross 806. 15 53.2 +13 12 STT 39 Ser. 15 53.6 -25 20 BU 36 2 Sco. 15 54.2 +16 59 A 2080 P = 110yr., a = 0.31", motion direct. 15 54.8 -50 20 DUN 195 B is CD-49@10123. 15 54.8 -54 34 RST 2984 A is the Cepheid SY Nor. 15 54.9 +34 22 STT 302 Proper motion of B -052 000. 15 54.9 -60 45 SLR 11 Variable? 15 55.0 -19 23 HU 1274 47 Lib. No duplicity seen 1923.5, 1924.5 (Van Biesbroeck). A is a spectroscopic binary. 15 55.1 -63 26 LDS 542 Beta TrA. 15 55.5 +10 06 STF 1986 Proper motion of B -009 +003. 15 55.5 -60 11 HJ 4813 Composite spectrum; G5II-III+A3. 15 55.7 -26 45 I 977 P = 158yr., a = 0.48", motion direct. 15 55.8 +37 57 H 94 H VI 94. Lambda CrB. 15 55.9 -02 10 STF 1985 A premature orbit has been computed. 15 56.2 +46 01 LDS 1429 Proper motion of B -015 +009. 15 56.5 +57 17 STF 1996 Proper motion of B -066 +097. 15 56.5 +15 40 STT Gamma Ser. Proper motion of A +312 -1281. 15 56.5 +03 25 BAL 2410 Proper motion of B -001 -136. 15 56.7 -34 26 COO 189 Spectrum of B may be K. Proper motion of B -015 -015. 15 56.8 +35 30 HJ 577 Proper motion of B -194 +078. 15 56.9 -29 13 SEE 251 Rho Sco. 15 56.9 -33 58 PZ 4 Xi (1) Lup. B is Xi (2) Lup. Proper motion of B +001 -03 15 57.1 -16 02 HJ 1281 The primary is variable. 15 57.2 +76 29 STF 2013 Proper motion of B +016 -046. 15 57.2 +05 09 WLF Wolf 611-612. 15 57.2 +03 24 STF 1987 Proper motion of B +005 +012. 15 57.6 +26 53 AGC 7 Epsilon CrB. 15 57.9 -31 58 HJ 4821 B is CD-31@12424. 15 58.7 -54 04 I 553 Spectrum composite: G9/K0III+A2V. 15 58.9 +21 47 STF 1990 B is BD+22@2906. Proper motion of B -031 -032. 15 58.9 -26 07 BU 622 Pi Sco. A is a spectroscopic and occultation binary. 15 59.1 -19 56 SHJ 213 B is BD-19@4274. Proper motion of B -019 -029, spectrum A8/9. 15 59.5 +25 55 JEF 2 The observation is doubtful. Others of same year do not suggest duplicity. This is the recurrent nova T CrB, with composite spectrum; sdBe+gM3+Q. 15 59.8 +17 23 STF 1994 These are the CD components of STF1993 at 15598+1723. 16 00.1 -38 24 RMK 21 Eta Lup. 16 00.3 -16 32 ENG 55 49 Lib. A is a long-period spectroscopic binary. 16 00.3 -22 37 LAB Delta Sco. A spectroscopic triple and occultation quad- ruple, with one pair resolved by speckle inter- ferometry: P = 10.58yr., a =0.107", motion direct. 16 01.0 +33 18 S 676 Rho CrB. 16 01.0 +01 47 LDS 4619 The primary is Wolf 622. 16 01.1 +28 08 AG 349 Spectrum is A7 (Yale) or K (McCormick). Proper motion of B -012 -011. 16 01.1 +26 10 H 75 H V 75. 16 02.4 +09 37 KU 109 B is BD+10@2944. 16 02.9 +60 41 STI 792 Proper motion of B -058 +002. 16 03.3 +36 38 BAG A spectroscopic binary with P = 108d. The inter- ferometer pair must be an additional component. 16 03.5 -57 47 SEE 258 Iota (1) Nor. P = 26.9yr., a = 0.37", motion retrograde. Proper motion of B -157 -095. 16 03.8 +04 59 KUI 69 43 Ser. 16 04.4 -11 22 STF 1998 Xi Sco. AB: P = 45.8yr., a = 0.76", motion direct. AB: Mt. Wilson spectral type F3s. 16 04.4 -11 27 STF 1999 AB: B is BD-11@4058. Proper motion of B -061 -033. Mt. Wilson spectral types G8 and K3. AD: D is AB of STF 1998. Physical. 16 04.8 +70 16 STT 143 B is BD+70@864. Proper motion of B +008 +027. 16 04.8 +60 03 STT 142 B is BD+60@1652. 16 05.0 -38 24 I 1081 Proper motion of B -017 -027 16 05.4 -19 48 BU 947 Beta (1) Sco. Common Proper motion with Beta (2) Sco. Speckle and occultation measures indicate a complex multiple system. H 7 H III 7. C is, Beta (2) Sco, and is a close interferometer pair found by McAlister. 16 05.6 +47 39 AG 202 Proper motion of B -002 +001 16 05.7 -06 17 FIN 384 Aa: A spectroscopic binary resolved by interferometry. P = 4.9yr., a = 0.066", motion retrograde. 16 05.7 -32 52 SEE 264 P = 114yr., a = 0.75", motion retrograde. Spectrum of C may be M. 16 06.0 +13 19 STF 2007 AB: B is BD+13@3063. Proper motion of B -017 -002. 16 07.2 -60 08 HJ 4829 One component is probably variable. Spectrum A5/7V+(M1/2). Proper motion of B -022 -023. 16 07.6 +29 00 STF 2011 Called Am by Bidelman. 16 07.6 -02 39 STF 2008 Proper motion of B -043 +014. 16 07.6 -12 45 BU 39 11 Sco. 16 07.7 +35 49 HJ 259 See ALI 370 at 16 07.4 +35 48. May be same star. 16 07.7 +20 22 WEI 30 Proper motion of B -048 +024. 16 07.7 -38 02 COO 193 Proper motion of B -048 -046. 16 08.0 -27 38 GLP 6 B is CD-27@10794. 16 08.1 +17 03 STF 2010 Kappa Her. B is BD+17@2965. Proper motion of B -021 -035. Mt. Wilson spectral types G4 and K1. 16 08.5 -10 06 BU 949 P = 55yr., a = 0.51", motion direct in a highly- inclined orbit. 16 08.6 -39 06 SEE 265 AB: A is the semiregular variable V856 Sco. There are indications of a 14d spectroscopic companion. There is an extended circumstellar atmosphere, and C shares common proper motion and radial velocity. 16 09.0 +57 56 ES 2651 A is a spectroscopic binary. 16 09.0 +36 29 BU 1087 Tau CrB. A is a spectroscopic binary. 16 09.2 -56 03 RST 1878 Spectrum composite; K0+A2. 16 09.6 -52 10 RST 813 CPD-51@8974. 16 09.7 -27 54 GLP 4 B is CD-27@10816. 16 10.2 -40 08 I 1082 Measures uncertain, too close. 16 10.3 +59 45 LDS 2370 BD+60@1658a. 16 10.5 +03 54 KU 110 Proper motion of B -027 +006. 16 10.6 +17 22 ROE 139 Star C is A of ROE at 16 10.7 +17 22. 16 10.7 -22 52 BRT 1496 CD-22@11390. 16 10.9 -10 06 WRH 24 Round 1959. 16 11.1 -08 14 MTL 1 Mitchell ascribed to STF 2012 rej. B is BD-07@4220. 16 11.8 +42 22 STF 2024 H IV 115. Composite spectrum; K4II+F6-8V. 16 11.8 +36 26 WRH 21 Single 1949, 1950. A long-period spectroscopic binary. 16 12.0 -19 28 CHR 146 Nu Sco. A is a spectroscopic and occultation binary. H 6 H V 6. Shows two spectra, B8V+B9VpSi, so the system is at least quintuple. 16 12.1 +14 33 STF 2017 B is BD+14@3011. Proper motion of B -013 +009. 16 12.1 +11 55 STF 2016 Proper motion of B +032 -012. 16 12.3 -28 25 HJ 4839 12 Sco. 16 12.4 -43 39 HJ 4837 B is CD-43@10607. 16 13.5 -54 38 HDO 254 Kappa Nor. 16 13.7 +46 38 A 1642 P = 186yr., a = 0.61", motion retrograde. 16 13.8 -01 47 ARG 75 Proper motion of B +030 +029. 16 13.8 -52 09 RST 5594 CPD-51@9079. 16 14.3 -03 42 BUP 164 Delta Oph. 16 14.3 -50 05 HJ 4838 B is CD-49@10426. 16 14.7 +33 52 STF 2032 Sigma CrB. P = 1000yr., a = 6.6", motion direct. A is a Delta Scuti-type variable, TZ CrB, and double-lined spectroscopic binary, P = 1.14d. It exhibits atmo- spheric and coronal activity, and radio flares. There is a distant, 633" physical companion, L 1490-24, mag. 12.31. 16 15.4 -49 16 BRT 882 CPD-48@8267. 16 15.4 -63 41 R 274 Delta TrA. Duplicity questionable. 16 15.6 -08 22 BUP 165 18 Sco. Optical. 16 15.6 -50 59 CPO 461 CPD-50@9115. 16 16.0 +07 21 STF 2026 P = 474yr., a = 2.46", motion retrograde. 16 16.5 -06 59 RST 3939 A is the Algol-type system SW Oph. 16 16.7 +29 09 SHJ 223 Upsilon CrB. Possible spectroscopic binary. 16 16.9 +01 13 A 2181 P = 339yr., a = 0.44", motion direct. 16 17.0 -53 42 I 987 P = 96yr., a = 0.39", motion direct. 16 17.5 +75 45 LDS 1844 Eta UMi. 16 18.2 -02 16 STF 2033 Proper motion of B +003 -005. 16 18.3 -04 42 BU 1452 Epsilon Oph. 16 19.3 -42 40 SEE 271 Lambda Nor. Direct motion. Half a revolution. 16 19.5 -30 54 BSO 12 A is a spectroscopic binary. B is CD-30@13040. Proper motion of B +075 +029. 16 19.7 +46 19 BU 1198 Tau Her. A is a Beta CMa-type variable. 16 19.8 +26 47 A 225 P = 44yr., a = 0.11", motion retrograde. 16 19.8 -50 09 HJ 4841 Gamma (2) Nor. 16 20.1 -20 03 SHJ 225 H V 134. B is BD-19@4358. Proper motion of B -013 -020. 16 20.3 -78 42 BSO 22 Delta (1) Aps, an irregular variable. B is CPD-78@1093, spectrum K3III. Proper motion of B -010 -032. 16 20.5 -20 07 B 1808 AB: Mt. Wilson spectral types B9,A0n. SHJ 226 AB-C: H V 124. Proper motion of C -006 -035. 16 20.9 +64 22 STF 2046 Proper motion of B -030 -031. 16 21.2 +22 59 HU 481 P = 192yr., a = 0.67", motion retrograde. 16 21.2 -25 36 BLM Aa: Sigma Sco. A is a Beta CMa-type variable with multiple periods, is a spectroscopic binary, and an occultation double. Composite spectrum; B2III+O9.5V. H 121 H IV 121. 16 21.9 +19 09 SHJ 227 Gamma Her. A is a spectroscopic binary. B is BD+19@2085. Proper motion of B -035 -041. 16 22.1 +30 54 CHR 53 Xi CrB. 16 22.4 +33 48 STF 29 AB: Nu (1) CrB. H 81 Aa: H N 81. H 18 Bb: H VI 18. Nu (1) and Nu (2) CrB. 16 22.4 -32 20 JSP 691 P = 106yr., a = 0.58", motion retrograde. 16 22.5 -04 15 BU 1453 B is BD-03@3930. Measured in connection with STF 3103rej. 16 22.5 -43 55 DUN 200 B is CD-43@10723. 16 22.9 +38 15 KU 53 Proper motion of B +011 -108. 16 22.9 +32 20 H 38 H V 38. Proper motion of B -010 -032. 16 22.9 -31 04 HJ 4847 Proper motion of B -016 +009. 16 23.4 +42 51 ARG 76 Proper motion of B -020 +017. 16 23.8 +61 42 CHR 138 The third component can not be associated with A for certain at this time. 16 23.9 -46 37 RST 843 CPD-46@7946. 16 24.0 +61 31 STT 312 Eta Dra. Both A and B are variable suspects. 16 24.0 +48 22 BUP 168 Distance 1128.4". 16 24.2 +37 02 STF 2044 Proper motion of B -105 -011. 16 24.5 -37 34 B 868 Measures uncertain, too close. 16 24.6 -48 13 HJ 4846 Proper motion of B -001 -021. 16 24.7 -29 42 H 39 H N 39. 16 24.9 -37 55 HJ 4852 Spectrum: A3/5II/III. 16 24.9 -52 05 BRT 891 CPD-51@9487. 16 25.3 -49 09 COO 197 A premature orbit has been computed. C is optical. 16 25.4 +37 24 CHR 55 25 Her. A shell star. 16 25.4 +14 02 BU 625 Omega Her. A is variable. Proper motion of C -017 -010. 16 25.6 -23 27 H 19 H II 19. Rho Oph. Spectrum of D: B3/4V. 16 26.2 +02 11 BAL 1915 BAL suspected both A and B to be closer pairs. 16 26.6 -51 58 RST 845 CPD-51@9530. 16 26.6 -52 05 CPO 473 Proper motion of B -037 -045. 16 26.8 +12 03 A 1859 Too close 1935 to 1945. Apparently a change of quadrant at this time. 16 26.9 +01 01 A 2233 Proper motion of B +007 -014. 16 27.1 +42 55 BU 815 See ADS for rectangular measures. Proper motion of D -011 -030. 16 27.2 -47 33 HJ 4853 Epsilon Nor. The primary is a spectroscopic binary. B is CD-47@10764. Proper motion of B -010 -026. 16 27.3 -43 46 I 565 Proper motion of B +052 -044. 16 27.8 -08 22 RST 3949 Upsilon Oph. A is a spectroscopic binary, P = 27.2d. 16 28.0 -64 03 DUN 201 Iota TrA. A is a spectroscopic binary. 16 28.4 +31 08 STF 2053 Proper motion of B -051 -004. 16 28.4 -61 08 B 1812 Alternative spectra: F5+A2. 16 28.8 -08 08 STF 2048 B is a spectroscopic binary. 16 28.9 +56 36 ARG 102 B is BD+56@1894. Proper motion of B -009 +029. 16 28.9 +18 25 STF 2052 P = 237yr., a = 2.28", motion retrograde. 16 29.4 +68 56 BU 356 Proper motion of B -041 +025. 16 29.4 +10 36 STF 2051 Proper motion of B 000 -016. 16 29.4 -26 26 GNT 1 Alpha Sco. A premature orbit has been computed. Composite spectrum; M1.5Iab-Ib+B4Ve. Variable. 16 30.1 +33 53 HU 1173 P = 98yr., a = 0.14", motion direct. 16 30.2 +21 29 BLA Beta Her. A is a long-period spectroscopic binary, resolved by speckle interferometry. 16 30.9 +01 59 STF 2055 Lambda Oph. P = 130yr., a = 0.97", motion direct. C is physical. 16 31.0 -46 29 HJ 4857 Spectrum of C may be M. 16 31.1 -16 37 BU 626 Phi Oph. 16 31.5 +08 18 SHJ 233 B is BD+08@3216. Proper motion of B +043 +077. 16 31.6 +19 17 STF 2057 C is A of STF 2058. Proper motion of B -054 -095. 16 31.6 +05 26 STF 2056 Proper motion of B -045 -027. 16 31.7 +17 04 H 3 H N 3. 16 31.8 +45 36 STF 2063 Proper motion of B -011 +042. 16 31.8 -02 16 A 693 P = 91yr., a = 0.20", motion retrograde. 16 31.8 -07 01 STF 3105 P = 540yr., a = 0.64", motion retrograde. 16 32.3 +00 12 HDO 308 Proper motion of B -016 -009. 16 32.6 +40 07 STT 313 Called G5II comp? by Bidelman. 16 32.7 +09 48 AG 350 Proper motion of B -008 -004. 16 32.9 -46 56 CPO 480 A is variable. 16 33.1 -60 54 DUN 203 B is CPD-60@6558. Proper motion of B +069 +078. 16 33.5 +30 30 BU 818 A is a spectroscopic binary. 16 33.9 -48 07 I 1588 Slightly variable. Central star of planetary nebula. 16 34.1 +42 26 LAB Sigma Her. Double-lined spectrum. Possibly ambiguous: P = 15.2 or 7.48yr., a = 0.11 or 0.074" motion retro- grade. 16 35.2 +37 21 PAR A is the Mira-type system W Her. 16 35.4 +17 03 WEB 6 A is a spectroscopic binary. B is BD+17@3054. Proper motion of B -028 -018. 16 35.4 -58 05 HU 1605 Spectrum of B may be M. 16 36.2 +52 55 STF 2078 17 Dra. Common proper motion with 16 Dra. STF 30 C is 16 Dra. 16 36.6 +69 48 BU 953 P = 185yr., a = 0.39", motion retrograde. D is physical. Proper motion of D -034 +044. 16 37.0 +69 49 BAZ 7 C is physical. 16 37.4 -61 33 HJ 4862 Proper motion of B +010 +011. 16 37.7 -30 57 HJ 4869 Proper motion of B +002 -030. 16 38.4 +35 14 COU 985 A premature orbit has been computed. 16 38.4 -43 24 HJ 4867 Proper motion of B +005 -026. 16 38.6 +38 20 STF 2080 See ADS for rectangular measures. 16 38.7 +48 56 STF 2082 42 Her. Proper motion of B -014 +025. 16 38.8 +13 41 STF 2071 Proper motion of B -005 -003. 16 39.1 +60 42 STF 2092 A is the Algol-type system WW Dra, P = 4.63d. Proper motion of B +008 -061. 16 39.6 +23 00 STF 2079 Proper motion of B +040 -029. 16 39.7 -57 00 HJ 4866 A is the Algol-type system R Ara. 16 40.1 +29 01 BU 42 Proper motion of B +007 +007. 16 40.5 +09 37 KU 113 Proper motion of B -001 -043. 16 40.6 +04 13 CHR 56 37 Her. B is 36 Her, BD+04@3234. 16 40.7 -00 09 STF 2076 Proper motion of B -039 -044. 16 40.9 -45 50 DON 806 CPD-45@8073. 16 41.3 +31 36 STF 2084 Zeta Her. P = 34.5yr., a = 1.36", motion retrograde. 16 41.3 +30 06 A 349 P = 126yr., a = 0.395", motion retrograde. 16 41.3 -48 46 MLO 8 AB: A is a spectroscopic binary. DUN 206 AC: C has variable velocity. 16 41.6 +44 28 L 14 Another measure: 1911.70, 119.1@, 19.96". Error in one of the distances? 16 41.6 +26 55 CHR 57 39 Her. A short-period (2.3d) double-lined spectro- scopic binary. Hence a triple. 16 41.9 -47 23 COO 199 B is CD-47@10952. 16 42.5 -37 05 R 283 Premature orbits have been computed. 16 42.6 +23 40 STF 2087 Proper motion of B -068 +040. 16 42.7 +13 36 STF 2083 Proper motion of B -039 -155. 16 42.9 +38 55 STF 2093 Eta Her. Aa in direction of C and 2/3 the distance. Fainter than C. 16 43.0 -60 56 HJ 4874 Proper motion of B 000 -010. 16 43.1 -77 31 HJ 4858 Beta Aps. 16 43.5 +20 43 STT 149 B is BD+20@3324. Proper motion of B +017 -004. 16 43.6 +06 37 H 127 H V 127. B is BD+06@3281. Proper motion of B +003 -001. 16 43.8 -53 30 FIN 251 Composite-like spectrum: B8/9(IV)+F/G. 16 43.9 +43 29 D 15 P = 121yr., a = 0.93", motion retrograde. 16 43.9 -00 32 GLP 12 Proper motion of C +061 -020 according to EBL. Possibly that of A? 16 43.9 -41 07 CPO 70 B is CD-40@10649. Proper motion of B -049 -019. 16 44.3 -00 33 STF 2086 Proper motion of B +002 -005. 16 44.4 -42 24 DUN 207 B is CD-42@11486. 16 44.7 -49 00 HJ 4882 CPD-48@8773. B is CPD-48@8774. 16 44.8 -39 12 DAW 71 CPD-38@6519. 16 45.0 +06 05 STT AB physical. Alternate specral type G3IV is more reasonable considering the magnitude difference. B has variable radial velocity. 16 45.3 +56 47 MCA 44 A spectroscopic triple with the wider pair, presumably, now resolved by speckle interferometry. 16 45.7 +30 00 STF 2098 C is BD+30@2872. Proper motion of C +023 +004. 16 45.8 +08 35 SHJ 239 43 Her. 16 45.8 -00 46 A 1141 Ambiguous case. P = 62 or 31yr., a = 0.23 or 0.11", motion retrograde. 16 46.0 +82 02 HDO 143 Epsilon UMi. A is an Algol-type system. 16 46.7 -67 07 HDO 257 Variable. 16 47.2 +02 04 STF 2096 19 Oph. A is a spectroscopic binary. Proper motion of B -008 -016. 16 47.2 -33 01 PRO 138 May be CD-32@12016. 16 47.5 -48 19 DUN 211 B is CD-48@11174. Proper motion of B +001 -037. 16 47.8 +05 15 BUP 174 45 Her. A is a spectroscopic binary, and is variable. 16 48.1 +05 00 BRT 2167 1896.4: Barton gave position angle 068@, mag.12.0-12.0. 16 48.2 -36 53 DUN 209 B is CD-36@10973. Proper motion of B +025 +009. 16 48.3 -28 45 HJ 4887 B is CD-28@12420. 16 48.7 -55 26 DUN 210 B is CPD-55@7693. 16 48.9 +59 30 STT 316 B is BD+59@1762. Proper motion of B -028 +012. 16 49.0 -19 36 HJ 4888 Proper motion of B +014 -097. 16 49.2 +45 59 BU 627 52 Her. A is an Alpha CVn-type variable, V637 Her. A 1866 BC: P = 57yr, a = 0.27", motion direct. 16 49.8 -59 02 RST 5067 Eta Ara. 16 49.9 -60 25 B 2393 Spectral type of A may be A. 16 50.1 +04 43 BUP 175 B is BD+04@3264. Proper motion of B -044 +005. 16 50.6 -50 03 COO 201 Composite spectrum; A5III+F7III. 16 50.9 -27 58 B 2820 A is the Mira-type variable BI Sco, and B is the Cepheid GW Sco. 16 51.1 +09 24 STF 2106 P = 1080yr, a = 1.25", motion retrograde. 16 51.1 -46 48 CPO 494 Proper motion of B -014 -010. 16 51.4 +01 13 STT 315 21 Oph. Premature orbits have been calculated. 16 51.4 +01 09 STF 2105 Proper motion of B -006 -009. 16 51.8 +28 40 STF 2107 P = 258yr., a = 0.98", motion direct. 16 53.0 +44 24 STT 317 AC: C is BD+44@2622. Proper motion of C +042 -005. 16 53.0 +31 42 BU 1454 53 Her. 16 53.2 -47 59 B 2398 Spectral type K? 16 53.4 +29 25 HEI 13 Proper motion of B -089 -070. 16 53.5 -60 49 B 2396 Spectral type M? 16 54.0 -41 48 B 1833 A spectroscopic binary. 16 54.0 -41 48 SEE 294 Variable in light and radial velocity. 16 54.0 -46 55 HJ 4890 B is CD-46@11089. Proper motion of B -007 -027. 16 54.2 -41 50 CPO 500 CPD-41@7737. 16 54.2 -41 50 SEE 297 Light and velocity variable. Spectroscopic binary, P=5.97d. 16 54.3 -41 49 B 1834 A is a Wolf-Rayet system, spectrum WC7+O5. 16 55.0 +25 44 STF 2110 56 Her. A is a spectroscopic binary. 16 55.2 +63 32 STF 2116 Proper motion of B -008 +028. 16 55.4 +18 26 BU 954 54 Her. 16 55.5 -08 20 KUI 75 Wolf 630. P = 1.72yr., a = 0.21", motion retrograde. A flare star, V1054 Oph. The radial velocities indicate a third component. The intrinsically very faint star VB 8 (mag. 17, 220") is also a member of the system. There is strong evidence that it is an astrometric binary. Wolf 629 (mag. 11.7, 72") is also physical, and is a spectroscopic binary, so that the whole system is probably a septuple. 16 55.5 -39 28 SEE 309 Proper motion of B -001 -005. 16 55.5 -39 29 SEE 308 CPD-39@7160. 16 56.4 +65 02 STF 2118 20 Dra. A premature orbit has been computed. 16 56.4 -41 04 CPO 501 Spectral type K? 16 56.6 +57 11 A 1143 P = 84yr., a = 0.23", motion retrograde. 16 56.6 +51 27 ES 2654 Proper motion of B +020 -035. 16 56.6 +45 05 ES 2655 B is BD+45@2469. 16 56.8 -23 09 BU 1117 24 Oph. 16 56.9 +15 40 HEI 71 There is a third star at 71 degrees, 31" (Heintz). 16 57.1 -19 32 SHJ 240 Proper motion of B -047 -050. 16 57.3 +86 51 STT 340 B is BD+86@263. Proper motion of B -028 +065. 16 58.2 -29 18 RST 1919 CPD-29@4538. 16 58.3 -33 37 I 1304 A is the Cepheid RV Sco. Also a spectrum variable. 16 58.9 -37 37 SEE 315 P = 38yr., a = 0.18", motion direct. 16 59.3 +65 13 STF 2124 Proper motion of B +013 +018. 16 59.9 -59 20 HJ 4900 B is CPD-59@6877. A is slightly variable. 17 00.3 +30 56 ISO 3 Epsilon Her. Spectroscopic binary, P = 4.02d. 17 00.3 -76 12 GLI 232 Spectrum of B: A8/F0. Proper motion of B -025 -026. 17 00.4 -48 39 SEE 316 Spectrum composite; G8-K0III+G. 17 00.5 +06 35 CHR 59 A spectroscopic binary. 17 01.0 +37 55 HJ 262 A pair of 12th magnitude stars in field p: 120.8@, 19.7". In the same field as HJ 263, BDS 7842. 17 01.1 -04 13 ENG 59 30 Oph. 17 01.3 -28 08 B 326 Retrograde motion. 17 01.6 +14 57 H 122 H IV 122. STF 2115. A is the Alpha CVn-type variable V451 Her. 17 02.0 +08 27 STF 2114 A spectroscopic binary. 17 02.4 -11 54 STF 3108 B is BD-11@4281. Proper motion of B +032 -027. 17 02.6 -55 04 HJ 4905 A is the semiregular variable T Ara. B is CPD-54@7976. 17 03.1 -53 14 HDO 263 Epsilon (2) Ara. Duplicity doubtful. 17 03.1 -58 33 I 997 Composite-like spectrum: A3/5V+K0III. 17 03.3 +59 35 STF 2128 Mt. Wilson spectral types K5 and M0. Proper motion of B -373 +250. 17 03.6 +69 48 A 1146 P = 155yr., a = 0.40", motion retrograde. 17 03.9 +53 14 STT 151 Proper motion of B +014 -054. 17 03.9 +19 41 BU 822 A spectroscopic binary. 17 03.9 -19 56 RST 3065 CPD-19@6092. 17 04.0 -51 05 DUN 212 B is CD-50@10977. 17 04.6 -38 00 B 890 CPD-37@6897. 17 04.8 -37 53 HJ 4915 Spectral type K? 17 05.0 -05 04 LDS 6317 AB: Wolf 531. B is BD-04@4226. Proper motion -957 -1135. 17 05.0 -51 22 RST 5596 CPD-51@10149. 17 05.3 +54 28 STF 2130 Mu Dra. P = 672yr., a = 3.94", motion retrograde. C is physical. BU 1088 AC: Mt. Wilson spectral types F5s. 17 05.4 +12 44 H 133 H V 133. 60 Her. Proper motion of B -004 -004. 17 05.4 -33 46 WNO 5 Spectral type of B may be M. Proper motion of B -004 -008. 17 05.6 -41 06 HLN 41 CPD. 17 06.2 -38 38 SEE 318 P = 224yr., a = 0.68", motion direct. 17 06.5 -02 36 STF 3110 Proper motion of B -031 -040. 17 06.6 +00 39 BU 823 P = 330yr., a = 1.18", motion direct. 17 06.9 -01 39 STF 2122 Proper motion of B +032 -028. 17 07.0 +06 48 STF 2123 Proper motion of B -006 -090. 17 07.5 +38 10 COU 1291 P = 59yr., a = 0.14", motion direct. 17 07.5 +35 57 HJ 264 This is A of HJ 264 and A of HU 1176. 17 08.0 +35 56 HU 1176 The speckle observations now resolve the former am- biguity: P = 8.13yr., a = 0.112", motion retrograde. 17 08.2 +01 43 AG 208 Proper motion of B +025 -020. 17 08.2 -01 05 A 1145 P = 150yr., a = 0.50", motion retrograde. A is a spectroscopic binary. 17 08.4 -44 43 CPO 71 Proper motion of B -017 +013. 17 08.7 +34 07 KU 115 Proper motion of B -030 +016. 17 08.8 +65 43 STA Zeta Dra. A premature orbit has been computed. 17 09.1 -37 53 B 896 CPD-37@6976. 17 09.7 +30 21 STF 2131 B is BD+30@2938. Proper motion of B +001 +018. 17 09.9 -82 19 HJ 4884 B is CPD-82@701. Proper motion of B +009 -021. 17 10.2 +54 30 STF 2138 B is BD+54@1862. Proper motion of B +104 -095. 17 10.4 -15 44 BU 1118 Eta Oph. P = 88yr., a = 0.86", motion retrograde in a highly-inclined orbit. 17 10.7 -44 33 I 1312 Spectrum composite; G8-K0III+G. 17 10.8 -60 21 B 1846 Spectrum: G8/K0III+A/F. 17 11.5 -16 30 HU 169 P = 103yr., a = 0.21", motion retrograde. 17 11.9 -01 51 LPM 629 P = 33.5yr., a = 0.69", motion direct. 17 12.1 +45 40 KUI 79 P = 12.95yr., a = 0.762", motion retrograde. Proper motion of A +257 -1565. 17 12.1 +21 14 STF 2135 Proper motion of B +020 +007. 17 12.5 +10 35 B 2826 37 Oph. 17 12.7 +23 52 POU 3262 Proper motion of B +008 -015. 17 12.9 +42 20 BUP 176 Proper motion of A -1040 -345. Proper motion of B -013 000. 17 13.0 -58 36 HJ 4920 A is a spectroscopic binary, P = 2.88d. 17 13.1 +54 08 STF 2146 AB: Proper motion of B -012 +097. 17 13.1 -25 32 RST 3076 Spectrum: B9/9.5IV/V. 17 13.3 -67 12 DUN 214 B is CPD-67@3295. 17 13.3 -72 43 HJ 4914 Composite-like spectrum: G5III+A4/5V. 17 13.6 +17 16 A 2087 P = 100yr., a = 0.29", motion direct. Ambiguous? 17 13.7 -54 25 R 294 B may be variable. 17 14.0 +16 21 HO 557 A is the W UMa-type system AK Her. 17 14.1 +56 08 STT 327 P = 90yr., a = 0.28", motion direct. 17 14.2 +19 19 STF 2139 This star has two distant companions nearly the same distance: 1904.26, 163.0@, 33.3". 17 14.2 +06 22 A 1147 Proper motion of B -006 +022. 17 14.5 -39 46 HJ 4926 A is the variable V915 Sco. 17 14.6 +14 23 CHR 139 Alpha Her. A premature orbit has been computed. A is a semiregular variable. B is a spectroscopic binary, spectrum composite; G5III+F2V. Proper motion of B -006 +031. 17 14.8 +10 00 STF 2143 Proper motion of B +003 -012. 17 15.0 +24 50 BNU Delta Her. AB is optical. A is a spectroscopic binary now resolved by speckle interferometry. 17 15.3 -26 36 SHJ 243 36 Oph. Proper motion -480 -1142. A premature orbit has been computed. A may be a spectroscopic binary. AC: Proper motion of C -481 -1134. C has common proper motion. 17 15.6 -10 18 BU 957 P = 98yr., a = 0.28", motion retrograde in a highly-inclined orbit. 17 15.6 -38 36 FIN 355 Rapid motion. 17 15.7 -09 49 A 2592 P = 128yr., a = 0.34", motion retrograde. 17 16.1 -25 56 RST 3082 Spectrum: B9.5/A0IV/V. 17 16.3 -42 20 I 408 A is variable. 17 16.5 +04 13 LDS 989 Wolf 661-2. 17 16.5 +01 13 HJ 854 A is the Algol-type system U Oph., spectrum composite; B5Vnn+B5V. 17 16.6 +26 35 WHC 15 Probable rapid motion in a highly-inclined orbit. 17 16.6 +04 40 LDS 4734 A is Wolf 664. 17 16.6 -00 27 A 2984 41 Oph. A premature orbit has been computed. 17 16.9 +89 02 HJ 2985 Lambda UMi. 17 17.3 +33 06 STT 328 68 Her. A is the Beta Lyrae-type system u Her. Composite spectrum, B1.5Vp+B5III. 17 17.3 -30 10 BU 1119 Spectroscopic binary. 17 17.3 -60 16 B 1853 Spectrum: G8/K1III+A. 17 17.4 -66 57 LDS 587 A is a spectroscopic binary, P = 1.68d. 17 17.7 -26 38 H 35 H I 35. Proper motion of B -009 -010. 17 17.8 +28 44 S 686 B is BD+28@2714. Proper motion of B +003 -035. 17 18.0 -24 17 H 25 Omicron Oph. H III 25. 17 18.4 +32 40 BU 628 A premature orbit has been computed. 17 18.4 +04 51 SCJ 14 B is BD+05@3367. 17 18.4 -32 23 COO 211 Proper motion of B +020 +005. 17 18.5 +53 46 ES 776 Heintz confirms that the Furner measures listed in ADS belong to this system. 17 18.6 +32 29 L 15 Lewis mentions a pair 2' s: 1900.5, 028@, 5.55". Position of L 15 revised by Heintz. 17 18.6 -32 23 PRO 154 CPD-32@4467. 17 18.7 +21 46 STT 152 B is BD+21@3090. 17 18.9 -24 00 H 54 H VI 54. 17 19.0 -34 59 MLO 4 P = 42.1yr., a = 1.82", motion retrograde. Spectrum composite; K3V+K5V. Proper motion +1167 -169. C is physical. Spectral type of C may be M. 17 19.1 -46 38 BSO 13 Premature orbits have been computed. Proper motion of A +1062 +158. 17 19.3 -53 23 DUN 215 B is CPD-53@8531. Proper motion of B -054 -079. 17 19.4 -44 13 HDO 269 Spectrum composite; B9.5V+A6III. 17 19.5 -50 04 FIN 356 Composite spectrum, F8III+B9V. 17 19.9 +26 29 OSV 5 Ross 867. Both components are flare stars, V647 and V639 Her. 17 20.0 +72 35 STF 2179 Proper motion of B -024 +084. 17 20.0 -06 26 STF 2149 Proper motion of B -007 -024. 17 20.0 -08 01 CHR 151 B is BD-07@4426. 17 20.7 +32 28 DOR 1 72 Her. Struve-Dorpat. Proper motion of A +137 -1041. Variable. 17 20.7 -07 06 A 2593 P = 73.5yr., a = 0.26", motion retrograde. 17 20.8 +01 56 LDS 6319 Wolf 672. Colors indicate white and red dwarf stars. 17 20.8 -12 51 SHJ 247 Nu Ser. B is BD-12@4724. Proper motion of B +021 +008. 17 20.9 +24 30 S 687 70 Her. A is a spectroscopic binary. 17 21.0 -21 07 DON 832 Xi Oph. 17 21.4 -37 07 BRT 1714 CPD-36@7238. 17 21.5 +28 45 CHR 194 Spectroscopic binary. 17 21.5 -56 28 HJ 4939 B is CPD-56@8164. 17 21.7 +39 58 MCA 47 P = 5.54yr., a = 0.072", motion direct. 17 22.1 +23 10 COU 415 p = 60yr., a = 0.28", motion retrograde. 17 22.1 -70 07 FIN 373 Iota Aps. 17 22.2 -59 02 HJ 4934 B is CPD-58@7077. 17 23.3 -47 28 HDO 271 Iota Ara. A is variable. 17 23.7 +37 09 MCA 48 Aa: Rho Her. Suspected of variable velocity, and resolved by speckle interferometry. STF 2161 Aa-B: Proper motion of B -040 000. 17 24.0 +38 35 HU 1179 P = 102yr., a = 0.16", motion retrograde. 17 24.0 -09 21 RST 3972 P = 14.73yr., a = 0.148", motion direct. 17 24.1 +03 04 STF 2158 Proper motion of B +001 +002. 17 24.3 -37 22 RST 3091 Spectrum: B8/9III/IV. 17 24.6 +39 13 S 689 B is BD+39@3124. Proper motion of B -005 +018. 17 24.6 +32 15 H 5 AB: H N 5. 17 24.6 -47 09 HJ 4944 B is CD-47@11509. 17 24.9 +13 20 STF 2159 Proper motion of B +008 -009. 17 24.9 -49 50 CPO 523 CPD-49@9962. 17 25.1 +34 44 HU 922 P = 110yr., a = 0.40 ", motion retrograde. 17 25.1 +03 48 BAL 2440 Proper motion of B -003 -086. 17 25.4 -56 23 HJ 4942 Gamma Ara. 17 25.5 +00 30 RST 5432 P = 147yr., a = 0.33", motion retrograde. 17 25.9 +16 55 KUI 81 A is the irregular variable V640 Her. 17 26.0 -50 38 HDO 313 Kappa Ara. 17 26.2 +29 27 STF 2165 Called a Delta Del-type star by Bidelman. 17 26.7 +31 05 LDS 995 B is BD+31@3025. 17 27.9 +11 23 STF 2166 B is BD+11@3183. Proper motion of B -031 +001. 17 27.9 -47 02 RST 5543 A light (V750 Arae) and velocity variable. 17 28.3 -20 58 A 2244 P = 45yr., a = 0.20", motion direct. 17 28.7 -23 04 RST 3103 CD-22@12047. 17 29.0 -43 58 DUN 217 Spectrum of B: A2IV. 17 29.0 -50 48 CPO 527 CPD-50@10113. 17 29.3 +29 24 A 351 AB: P = 60yr., a = 0.60", motion direct, highly- inclined. KUI 82 AB-C: Proper motion of C -006 -004. The Baize measures seem to need addition of one revolution of the screw. 17 29.5 +34 56 STF 2178 BDS 8092. H III 40 may be same star. Proper motion of B -031 +015. 17 29.7 -17 48 HJ 2806 Proper motion of B -011 -035. 17 29.9 -01 18 STF 2172 Proper motion of B +024 +013. 17 30.1 -33 43 HWE 39 A is a spectroscopic binary, P = 38.10d. 17 30.4 +52 18 BU 1090 Beta Dra. 17 30.4 -01 04 STF 2173 P = 46.4yr., a = 0.98", motion retrograde in a highly-inclined orbit. 17 30.8 +03 49 A 2247 Round in 1918. In 1923, 183@, 0.1". Quadrant doubtful. Round 1957, 1958. Visible in 1978. 17 30.8 -37 26 B 912 P = 105yr., a = 0.235", motion direct. 17 31.1 +10 27 STF 2176 Proper motion of B +003 -006. 17 31.1 -60 41 HJ 4951 Delta Ara. 17 31.4 +02 43 A 2386 Single 1957-1964. Possibly not double. 17 31.5 -60 26 I 600 P = 611yr., a =0.49", motion retrograde. 17 31.8 -46 02 I 40 Proper motion of B -002 -025. 17 31.8 -49 53 HJ 4955 Alpha Ara. A spectroscopic binary. 17 32.0 +68 08 BU 1458 27 Dra. A is a spectroscopic binary. 17 32.0 +02 49 STT 331 This is a measure of a faint pair 1 minute preceding STT 331. 17 32.2 +55 11 STF 35 Nu (2) Dra. Proper motion of B +147 +057. B is Nu (1) Dra., BD+55@1944. Both components are spectroscopic binaries. 17 32.2 +11 56 ISO 4 A spectroscopic binary, P = 6.8d. 17 32.4 +28 48 A 352 P = 61yr., a = 0.17", motion retrograde. 17 32.6 +34 45 HU 1181 P = 24yr., a = 0.18", motion direct. 17 33.4 +74 14 LDS 1871 B is BD+74@718. 17 33.6 -35 47 BRT 1725 CPD-35@7036. 17 33.6 -37 06 SEE 334 Lambda Sco. Variable. Spectroscopic binary. 17 34.2 -19 10 B 1863 Measures uncertain, too close. 17 34.6 +09 35 STF 34 53 Oph. B is BD+09@3423. 17 34.6 -52 56 CPO 533 B is CPD-52@10710. 17 34.7 -32 35 HJ 4962 Central star of cluster NGC 6383, and a spectroscopic binary, P = 3.37d. 17 34.8 -11 15 HJ 4964 B is BD-11@4410. Proper motion of B +009 +002. 17 35.0 +61 53 BU 962 26 Dra. P = 76yr., a = 1.52", motion retrograde. There is a distant common proper motion companion at 740". 17 35.7 +04 09 A 2985 Round 1956, 1958, 1960. Retrograde motion. 17 36.0 +21 00 STF 2190 A is a spectroscopic binary. Proper motion of B +011 -016. 17 36.0 +20 34 HJ 2807 Probably identical with BDS 8082, STF 2190. 17 36.0 -20 25 BHA 19 CPD-20@6597. 17 36.2 +54 25 ES 637 B is BD+43@2775. 17 36.2 +06 37 STF 2188 Proper motion of B +009 -004. 17 36.2 -33 30 B 914 Spectral type may be M. 17 36.2 -55 38 HJ 4959 B is CPD-55@8221. 17 36.4 +68 20 CHR 62 Aa is also the astrometric binary Cin 2354. Proper motion of A -351 -1266. ENG 61 Aa-B: B is BD+68@947. Proper motion of B +024 +101. 17 36.6 +07 23 A 1156 P = 209yr., a = 0.32", motion retrograde. 17 36.8 -20 57 HU 751 Direct motion. 17 37.0 +68 45 FOX 203 Omega Dra. A is a spectroscopic binary. 17 37.1 -16 36 BHA 58 Proper motion of B -021 -011. 17 37.2 +27 54 KUI 83 P = 24yr., a = 0.27", motion retrograde. C is physical. 17 37.5 +24 19 CHR 63 79 Her. 17 37.6 -15 24 ISO 6 Xi Ser. Aa is a spectroscopic binary, P = 2.29d. The Isobe pair is not the spectroscopic binary. 17 37.9 -37 52 I 247 A spectroscopic binary. 17 38.0 -48 37 CPO 542 Heintz reverses the quadrant. 17 38.4 -59 56 HJ 4961 B is CPD-59@7089. 17 38.6 +55 46 STF 2199 A premature orbit has been calculated. 17 38.7 +03 49 BAL 2445 Proper motion of B +013 +009. 17 38.9 +84 03 STF 2299 B is BD+84@397. 17 39.1 +02 02 SHJ 251 Spectroscopic binary. Composite spectrum, K0III+F4IV. 17 39.2 -51 12 HJ 4965 B is CD-51@11033. 17 39.4 +01 03 GIC Ross 534. 17 39.4 -15 46 HU 181 P = 144yr., a = 0.51", motion direct. 17 39.5 +46 00 BLA Iota Her. A is a spectroscopic binary, now resolved by speckle interferometry. BU 1459 Aa-B: Proper motion of B -005 +001. 17 39.7 +72 56 H 41 H I 41. 17 39.8 +59 08 ARG 103 Proper motion of B +011 +005. 17 39.8 -04 58 STF 2191 B is BD-04@4324. 17 40.0 +40 46 ES 1556 ES 1556a. 17 40.0 -00 38 BU 631 P = 147.5yr., a = 0.22", motion retrograde. 17 40.5 -20 45 DON 856 CPD-20@6623. 17 40.7 +31 17 STT 157 B is BD+31@3077. Proper motion of B -011 -018. 17 41.1 +24 31 STF 2194 Spectroscopic binary. Composite spectrum K0III+F4IV. Proper motion of B -020 +053. 17 41.1 -37 39 JSP 933 CPD-37@7379. 17 41.2 +41 39 STF 2203 BDS 8128, STT (App) 158 probably same star. 17 41.3 +61 36 STF 2219 Proper motion of B +009 +033. 17 41.8 -54 02 HJ 4969 B is CPD-53@8734. 17 41.9 +72 09 STF 2241 Psi (1) Dra. B is BD+72@805. Proper motion of B +017 -279. A premature orbit has been computed. 17 42.0 +15 57 BU 1251 P = 123 yr., a = 1.00", motion retrograde. The companion at 155" shares common proper motion. 17 42.0 +08 14 STF 2193 Proper motion of B +019 -020. 17 42.5 +24 34 ENG 62 83 Her. 17 42.7 -57 40 RST 5544 Spectral type of A may be G5. 17 43.2 -29 56 ARG 30 B is CD-29@13894. 17 43.3 +43 45 STF 2214 Proper motion of B +010 -001. 17 43.3 -57 43 I 377 A is the semiregular variable V Pav, P = 225d. 17 43.6 +34 46 STT 334 Proper motion of B +005 -015. 17 44.3 +14 25 HJ 1303 A is the eclipsing binary V624 Her. 17 44.3 -72 13 HDO 275 P = 101yr., a = 0.65", motion retrograde. 17 44.4 +02 58 STF 2201 Proper motion of B -018 +001. 17 44.6 +02 35 STF 2202 61 Oph. A is a spectroscopic binary. B is BD+02@3391. Proper motion of B +012 +013. 17 44.7 -42 44 FIN 341 Appears to be in rapid motion. 17 44.9 +31 08 STF 2213 Proper motion of B -012 000. 17 44.9 -18 39 A 2250 A is the semiregular variable SZ Sgr. 17 45.0 -16 46 VOU 42 Spectrum: Fm Delta Del. 17 45.0 -45 11 HJ 4973 B is CD-45@11856. 17 45.2 +51 57 STF 2225 AB: Proper motion of B -019 +043. CD: Proper motion of D -003 -003. 17 45.7 +17 43 STF 2205 A premature orbit has been computed. 17 45.9 +21 53 STT 335 B is BD+21@3209. Proper motion of B -008 +011. 17 46.0 +39 19 STF 2224 A is a spectroscopic binary. Composite spectrum, K3III+ F7V. It is also variable, V826 Her. 17 46.1 +05 32 CHR 157 In IC 4665. 17 46.1 -32 04 LDS 611 B is CD-32@13297. 17 46.4 -13 18 STF 2204 Proper motion of B -005 +006. 17 46.5 +27 43 STF 2220 AB: Mu Her. A is physical, and is a large-amplitude astrometric binary, P = 65yr. AC 7 BC: P = 43.2yr., a = 1.36", motion direct. 17 46.7 +14 47 STF 2217 Proper motion of B -025 +007. 17 46.7 -01 13 STF 2211 Proper motion of B -031 000. 17 46.8 +05 34 A 1161 In IC 4665. 17 47.0 +05 42 STF 2216 Proper motion of B +006 +003. 17 47.1 +47 37 CHR 64 A spectroscopic binary, P = 2.8d. Hence triple. 17 47.1 +17 42 STF 2215 A spectroscopic binary. A premature visual orbit has been calculated. 17 47.1 -38 07 I 1336 P = 36yr., a = 0.15", motion direct. 17 47.6 -26 22 J 1732 CPD-26@5975. 17 47.6 -40 08 SEE 338 Iota (1) Sco. A is a spectroscopic binary. 17 47.8 -22 11 B 358 CPD-22@6444. 17 48.3 -35 25 JSP 732 CPD-35@7269. 17 48.7 +01 10 STF 2221 Proper motion of B +006 +005. 17 48.9 -22 19 BRT 1508 CD-22@12253. 17 49.0 +04 58 STF 2223 Proper motion of B +003 -028. 17 49.0 +37 04 COU 1145 P = 20.70yr., a = 0.179", motion retrograde. 17 49.1 +50 47 CHR 65 30 Dra. 17 49.2 -36 18 JSP 734 CPD-36@7625. 17 49.6 -20 00 HJ 2810 AB: The CPD identifications of A and B are -19@6275 and -19@6274. 17 50.0 +41 57 STF 2237 Proper motion of B +022 -036. 17 50.2 -40 05 HDO 279 Iota (2) Sco. 17 50.3 +04 15 HJ 855 Proper motion of B +008 -005. 17 50.4 -36 52 JSP 737 CPD-36@7660. 17 50.5 -48 17 HJ 4982 B is CD-48@12074. 17 50.5 -53 37 HJ 4978 A is the Algol-type system V539 Ara. 17 50.6 +07 14 STT 337 A premature orbit has been computed. 17 50.7 +07 55 STF 2230 B is BD+07@3483. 17 50.7 -34 44 BRT 1741 CPD-34@7161. 17 50.9 -33 42 HDO 280 A is the Cepheid RY Sco, spectrum also variable. 17 51.4 +59 38 ROE 17 Proper motion of B -011 +041. 17 51.8 -13 36 HU 188 Spectrum: B9.5III/IV. 17 52.1 +01 07 S 694 B is BD+01@3525. Proper motion of B +011 +006. 17 52.3 +40 57 A 699 Too close 1928, 1932, 1957, 1960. 17 52.7 -07 57 STF 2234 Proper motion of B +009 -052. 17 53.0 +83 54 STT 349 P = 433yr., a = 0.64", motion direct. 17 53.0 -02 15 STF 2235 Proper motion of B +003 +014. 17 53.0 -07 55 STF 3128 P = 260yr., a = 0.94", motion retrograde. 17 53.1 +14 01 HJ 1306 Proper motion of B +002 +003. 17 53.3 +40 00 BU 130 90 Her. 17 53.3 +24 59 A 235 P = 37.4yr., a = 0.27", motion direct. 17 53.3 -34 44 BU 1123 A premature orbit has been computed. 17 53.3 -35 47 BRT 3325 CPD-35@7400. Neither this, nor the preceding Barton pair, BRT 3324, were found by Heintz. 17 53.4 +10 58 STT 160 B is BD+10@3314. 17 53.4 -26 39 HJ 4991 B is CD-26@12487. 17 53.4 -34 54 SEE 342 Spectroscopic binary. 17 53.5 +56 52 LDS 1457 Xi Dra. 17 53.6 -34 45 B 362 CPD-34@7283. 17 53.9 -34 45 B 1871 One component is a Beta Lyrae-type system, V906 Sco. 17 54.2 +11 08 FIN 381 P = 8.92yr., a = 0.087", motion retrograde. Called a spectroscopic binary in the Bright Star Catalogue; this may be motion in the visual pair. 17 54.3 -18 28 A 2253 Not seen 1927, 1934. Single 1958. 17 55.7 -24 56 J 2194 May be CD-24@13632. 17 55.7 -30 34 I 1011 Spectrum: B9.5II/III. 17 55.9 -70 32 HJ 4976 B is CPD-70@2439. 17 56.0 -66 32 HJ 4983 B is CPD-66@3163. 17 56.3 +02 59 A 2189 P = 150yr., a = 0.22", motion direct. 17 56.3 -15 49 HJ 2814 B is BD-15@4723. Proper motion of B -007 -059. 17 56.3 -32 28 JSP 748 A is the eclipsing binary V453 Sco, P = 12.61d. 17 56.4 +18 20 MCA 49 Proper motion of B 000 -016. 17 56.5 -34 08 JSP 934 CPD-34@7399. 17 56.6 +58 13 ES 20 A is the Mira-type variable T Dra, BD+58@1772a. 17 56.6 +51 29 BU 633 Gamma Dra. A is variable. 17 56.8 -37 55 JSP 751 CPD-37@7662. 17 56.9 +18 11 J 1352 J notes ADS positions are 1970 and 1920 (JO 27,80). In JO 35, 53 J uses 1950 ADS position and has a note " two couples?" And there is a measure that indeed looks different: 1951.62, 39.9@, 3.33", 11.3-11.3. 17 56.9 -35 14 BRT 1744 CPD-35@7528. 17 57.1 +00 04 STF 2244 P = 280yr., a = 0.71", motion direct. 17 57.2 +35 41 POP 10 HO 73? 17 57.2 +24 00 MCA 50 A spectroscopic and interferometric binary, now resolved. P = 2.4yr., a = 0.083", motion direct. 17 57.3 -52 12 HJ 4994 B is CPD-52@10926. Proper motion of B +001 -002. 17 57.4 +51 11 ES 78 Fox also notes a 1" double (12 mag.) 23" from A in 199@. 17 57.4 -35 08 JSP 753 CPD-35@7547. 17 57.5 +10 58 BU 1299 P = 256yr., a = 0.42", motion direct. 17 57.8 +27 51 ALL 2 Proper motion of B +034 +057. 17 57.9 -19 21 RST 5097 CPD-19@6357. 17 58.1 +52 13 STF 2261 Proper motion of B +011 -018. 17 58.3 -38 10 I 1347 I 1347 1/2. 17 58.4 +04 28 KUI 84 P = 14.6yr., a = 0.17", motion direct in a highly- inclined orbit. In the same field with Barnard's Star. Two astrometric mass-ratio determinations showed B to be twice as massive as A. This has now been confirmed by Tokovinen, who finds B to be a spectroscopic binary, P = 34.5d. 17 58.7 -22 32 B 367 CPD-22@6498. 17 58.9 -28 50 B 2848 CPD-28@6088. 17 58.9 -36 52 DUN 219 B is CD-36@12058. Proper motion of B -037 -048. 17 59.0 +02 59 BAL 2462 J 2119. The close pair suspected by BAL is not confirmed. 17 59.0 +02 02 STF 2252 C is BD+02@3444. Proper motion of C -010 -006. 17 59.1 +32 28 HU 1185 P = 131yr., a = 0.22", motion direct. 17 59.0 +30 03 STF 2259 Proper motion of B +010 +002. 17 59.1 -30 15 PZ 6 A is variable. Proper motion of B +034 -009. 17 59.1 -35 59 JSP 758 CPD-35@7594. 17 59.2 +64 09 STF 2273 Proper motion of B +012 +007. 17 59.2 -36 56 HJ 5000 A is the Algol-type system V1647 Sgr. 17 59.4 -17 24 RST 3144 A is the Algol-type system WX Sgr. 17 59.6 +43 14 COU 1784 Proper motion of B -003 +021. 18 00.2 +80 00 STF 2308 41 Dra. Spectroscopic binary, P = 1247.2d, with the highest known eccentricity to date, e = 0.975. B is BD+79@570, 40 Dra. Proper motion of B +046 +139. It is also a spectroscopic binary, P = 10.53d. 18 00.2 +08 51 STT 161 B is BD+08@3556. Proper motion of B -033 +027. 18 00.3 +21 54 A 1374 Angle decreasing. 18 00.5 -37 42 I 230 CPD-37@7765. 18 00.6 +02 56 BU 1124 67 Oph. H 2 H VI 2. 18 00.9 +26 33 STF 2263 Proper motion of B +010 -009. 18 01.0 +35 58 POP 110 Codiscovered by Olevic. 18 01.4 +84 36 HU 65 Proper motion of B -039 +016. 18 01.5 +21 36 STF 2264 95 Her. Proper motion of B +008 +028, spectrum G8III. 18 01.5 +03 31 BU 1202 Proper motion of C -003 +009. Proper motion of E +005 -009. 18 01.5 -36 12 BRT 1750 CPD-36@7919. 18 01.5 -37 32 JSP 763 CPD-37@7798. 18 01.8 +01 18 BU 1125 68 Oph. A spectroscopic binary. 18 02.2 -36 16 BRT 1751 CPD-36@7937. 18 02.4 -23 02 H 40 AB: H N 40. Proper motion of B +005 -008. H 6 AC: H N 6. 18 02.5 +44 14 BU 1127 A premature orbit has been computed. L 28 is probably the same star (Van Biesbroeck). 18 02.5 +26 19 HO 564 BU measured BD+26@3146, 26s preceding and 4' south of HO 564: 1905.8, 185.4@, 23.22", 8.3-11.5. 18 02.8 +01 37 BU 635 C is BD+01@3566. Proper motion of C -001 -006. 18 02.9 +56 26 STF 2278 AB: The BD numbers of A and B may be reversed. D is reversed. 18 03.1 +48 28 STF 2277 Mt. Wilson spectral type of B is G8. Proper motion of B +010 -004. 18 03.1 -08 11 STF 2262 Tau Oph. P = 280yr., a = 1.49", motion direct. A is a spectroscopic binary. 18 03.2 +07 55 STT 164 B is BD+07@3536. Proper motion of B +003 -015. 18 04.0 +39 23 L 19 Not found by B in 1958. 18 04.0 -01 35 BAL 579 Proper motion of B -007 -013. 18 04.1 +06 28 STF 2265 Proper motion of B +004 -021. 18 04.3 +42 06 COU 1786 Ambiguous case. P = 40.6 0r 18.75yr., a = 0.13 or 0.10", motion direct. 18 04.3 -40 19 WG 222 CPD-40@8381. 18 04.4 +03 29 STF 2266 Proper motion of B -021 -095. 18 04.4 -59 53 RST 5099 P = 46yr., a = 0.27", motion direct. 18 04.6 +50 53 STF 2279 Proper motion of B +012 +063. 18 04.6 -17 02 HU 194 Spectrum: Fm Delta Del. 18 05.0 +41 57 ROE 1 A is a spectroscopic binary. 18 05.0 -29 35 BLM Gamma (1) Sgr. A is the Cepheid W Sgr, spectrum also variable. It is a long-period spectroscopic binary and speckle and occultation pair. 18 05.1 -40 40 CPO 571 CPD-40@8400. 18 05.3 +81 29 STF 2326 B is BD+81@618. Proper motion of B +023 +034. 18 05.5 +02 30 STF 2272 70 Oph. AB: P = 88.3yr., a = 4.56", motion retrograde. Spectral types K0V, K4V. Proper motion of A +227 -1093. 18 05.7 +12 00 STF 2276 A is a spectroscopic binary, and B is a variable of the Beta CrB-type. Proper motion of B -007 -015. 18 05.7 -34 37 HJ 5012 B is CD-34@12450. Proper motion of B +053 +003. 18 05.8 +21 27 STT 341 P = 20.1yr., a = 0.25", motion direct. Also a Beta Lyrae-type system, V772 Her, P = 0.88d. C is physical. G is BD+21@3301. Proper motion of G -003 -003. 18 06.0 +04 34 STT 165 B is BD+04@3594. Proper motion of B +021 -001. 18 06.1 +34 50 POP Codiscovered by Popovic and Olevic. 18 06.1 -21 35 J 1736 CPD-21@6594. 18 06.3 +38 24 HU 1186 P = 103yr., a = 0.30", motion direct. 18 06.3 +28 43 HJ 1313 Pair measured by Bigourdan: 310.9@, 8.68". Not found by Doolittle. 18 06.4 -41 45 HJ 5011 B is CD-41@12402. 18 06.5 +09 20 HZG B is BD+09@3560. Proper motion of B -006 +005. 18 06.7 +13 59 AG 358 Proper motion of B -024 -038. 18 06.8 -43 25 HJ 5014 P = 191yr., a = 1.06", motion retrograde. 18 07.0 +30 34 AC 15 99 Her. P = 55.6yr., a = 1.08", motion direct. 18 07.1 +49 43 STT 344 A is a spectroscopic binary. 18 07.1 -49 49 I 1350 I 1350a. 18 07.3 +09 34 STT 342 72 Oph. Spectroscopic binary. 18 07.4 -30 11 B 1350 Spectrum: B9.5/A0IV/V. 18 07.5 +45 52 KUI 85 Nova Herculis. Not a true visual double star, but the system contains the eclipsing binary DQ Her. 18 07.5 +28 46 STA Omicron Her. A spectroscopic and interferometric binary. 18 07.5 +19 40 STT 524 P = 419yr., a = 0.43", motion retrograde. 18 07.8 +26 06 CHR 67 100 Her. Proper motion of B -006 +029. One component is variable. 18 07.8 +13 04 H 74 H V 74. 18 08.0 -16 37 RST 3996 There has been a large change, angle decreasing, in the unobserved interval 1951-1990. 18 08.8 +20 49 AGC 8 102 Her. A is a suspected spectroscopic binary. 18 08.9 -25 28 WNO One component is a Beta Lyrae-type system, V3792 Sgr. 18 09.1 +31 01 BLL 31 A is the Mira-type system T Her. B is BD+31@3185. Proper motion of B +004 -002. 18 09.2 -22 11 RST 3157 P = 9.4yr., a = 0.22", motion direct. 18 09.3 +59 45 STF 2300 Proper motion of B -005 +014. 18 09.6 +04 00 STF 2281 73 Oph. P = 286yr., a = 1.18", motion retrograde. 18 09.9 +03 07 BU 637 A is a spectroscopic binary. 18 10.0 -48 52 HJ 5017 B is CD-48@12312. 18 10.1 +16 29 STF 2289 A premature orbit has been computed. 18 10.2 +34 02 STF 2291 Proper motion of B -003 +010. 18 10.3 +21 28 BRT 2442 A third star at 62 degrees, 17" (Heintz). 18 10.4 +02 32 STF 2288 Proper motion of B -013 +001. 18 10.6 -16 45 S 700 Proper motion of B +005 +006. A 4th star "nearly south". 18 10.6 -75 11 HJ 4999 Proper motion of B -003 -014. 18 10.7 -40 32 HJ 5025 B is CD-40@12231. 18 11.1 +53 30 AG 217 Proper motion of B -018 +023. 18 11.2 -17 23 RST 3161 Composite spectrum G5+A0. 18 11.2 -19 51 BU 132 Same as SEE 501. A third component is indicated by lunar ioccultation. 18 11.2 -45 57 HDO 286 Epsilon Tel. 18 11.7 -23 42 HJ 5030 11 Sgr. 18 11.8 +33 27 B 2545 Called a spectroscopic binary. Variation undoubtedly due to motion in the visual orbit. Possibly ambiguous case: P = 24 or 58yr., a = 0.062 or 0.116", motion direct. 18 12.0 +51 10 AG 359 Proper motion of B +016 +039. 18 12.8 -16 18 HJ 2821 Spectrum: B5/7II/III. 18 13.0 +42 51 ES 473 B is BD+42@3026. Proper motion of B -013 +014. 18 13.0 +28 15 H 93 H V 93. B is BD+28@2956. Proper motion of B +010 +130. 18 13.0 +22 32 HJ 2825 Proper motion of B -007 -002. 18 13.0 -27 04 J 2199 CPD-27@6260. 18 13.2 +10 53 ROE 121 Proper motion of B +015 -013. 18 13.3 -44 10 BRT 1031 CPD-44@9008. 18 13.8 -21 04 H 7 H V 7. Mu Sgr. A is an Algol-type system and occultation binary. 18 14.0 -20 52 J 1622 CPD-20@6887. 18 14.1 -22 01 BRT 1520 CD-22@12732. 18 14.2 +64 45 COM 4 B is BD+64@1251. 18 14.4 +21 27 HJ 2828 B is BD+21@3356. Proper motion of B -044 -060. 18 14.6 +23 35 HU 318 Proper motion of B -006 +004. 18 14.6 +00 11 STF 2294 P = 278yr., a = 0.67", motion retrograde. 18 14.6 -47 22 HJ 5031 B is CD-47@12140. 18 14.7 +56 35 BU 1274 A is a spectroscopic binary. 18 14.7 -19 39 J 1623 CPD-19@6670. 18 14.8 -04 41 HJ 856 B is BD-04@4423. 18 15.0 -19 55 HJ 2823 B is BD-19@4922. 18 15.0 -50 18 I 429 Measures scattered, but probable rapid motion. 18 15.2 -20 23 BU 286 16 Sgr. A is a spectroscopic binary. 18 15.4 -48 51 HJ 5033 Proper motion of B +006 +029. 18 15.5 -18 40 SEE 349 Component not seen in 1934 with 36-inch. 18 15.7 +24 00 STF 2301 Proper motion of B -004 +003. 18 15.7 -63 03 HJ 5024 B is CPD-63@4344. 18 15.8 +41 07 ES 1651 A is the Beta Lyrae-type system TZ Lyr, P = 0.52d. 18 15.9 -27 16 J 2201 CPD-27@6313. 18 16.0 -53 33 HJ 5453 HJ 5453a. 18 16.2 +04 34 STT 167 B is BD+04@3677. Proper motion of B -020 +024. 18 16.3 -22 53 BRT 1522 CD-22@12777. 18 16.5 -27 48 RST 2043 CPD-27@6328. 18 16.6 -20 33 MCA 51 17 Sgr. 18 17.2 +51 03 AG 220 Proper motion of B +015 +004. 18 17.4 -19 20 B 2863 CPD-19@6748. 18 17.5 +29 31 COU 814 Proper motion of B 000 -013. 18 17.5 -16 39 HJ 2829 Spectrum: B2/3II/III. 18 17.6 +26 59 HJ 1317 The three measures by Bigourdan were not found, and so were omitted from this catalog. 18 17.6 -34 06 HJ 5036 A is the Algol-type system RS Sgr. 18 17.6 -36 46 BU 760 Eta Sgr. A is an irregular variable. 18 17.8 +43 51 A 578 P = 250yr., a = 0.26", motion retrograde. C is probably physical. 18 17.8 -16 58 WHC 16 This may be same star as BDS 8452, HJ 2826. 18 18.7 -18 37 BU 639 There was a close approach around 1900. 18 19.6 -19 44 WRH SEE 501 is probably BU 132. 18 19.7 +10 16 HU 197 P = 126yr., a = 0.46", motion retrograde. 18 19.7 +02 07 AG 219 Proper motion of B -064 +048. 18 20.2 -36 01 BRT 1769 CPD-36@8160. 18 20.4 -10 11 HER A post-T Tauri star, FK Ser. 18 20.5 -53 44 FIN 264 Spectrum: G0/5III+A7/F0. 18 20.8 +71 20 STT 353 Phi Dra. A premature orbit has been computed. A is an Alpha CVn-type variable and spectroscopic binary. 18 20.9 +03 23 HJ 5495 74 Oph. 18 21.0 -01 01 VKI LP 630-1. 18 21.0 -29 50 SEE 350 Delta Sgr. 18 21.1 +72 44 LAB Chi Dra. An astrometric, interferometric, and spectroscopic binary. 18 21.1 -13 39 RST 4585 RST 4585a. 18 21.3 -02 54 STF 8 Eta Ser. 18 21.6 +09 19 J 2515 J gives position angle 187@ in 1943. 18 22.0 -22 33 J 2208 CPD-22@6959. 18 22.2 -55 34 DUN 220 B is CPD-55@8630. Proper motion of B +075 -003. 18 22.4 +45 45 A 700 Round 1951-1954. Possible quadrant change. 18 22.9 +14 58 HU 581 P = 60yr., a = 0.22", direct motion in a highly-inclined orbit. 18 22.9 +08 35 ROE 99 Proper motion of B +003 -017. 18 23.2 -61 30 GLE 2 Xi Pav. A is a long-period spectroscopic binary. 18 23.6 -26 10 HO 566 If the quadrants are correct, a revolution has been completed. 18 23.7 +21 46 STT 109 Her. 18 23.7 +08 29 ROE 100 Proper motion of B +017 -022. 18 23.9 +58 48 STF 2323 39 Dra. A is a double-lined spectroscopic binary. C is physical, and is a spectroscopic binary, P =2.71d. 18 24.0 +38 44 HO 432 HO also notes an 11th magnitude star 100" in 44@ from A. 18 24.1 +01 30 HJ 858 Proper motion of B -015 -020. 18 24.1 -17 34 J 2127 Jonckheere gives angle as 40@ in his 1962 catalog. 18 24.2 -34 23 SEE 351 Epsilon Sgr. Infrared excess and probable circum- stellar disk. Spectral peculiarities lead to classi- fication problems. Alternative types B9IVp, A0II(shell). 18 24.3 -44 07 DUN 221 B is CD-44@12570. 18 24.7 -06 36 STF 2313 Proper motion of B -065 -041. 18 25.0 +27 24 STF 2315 P = 248yr., a = 0.63", motion retrograde. A is a spectroscopic binary. AC: 1898 distance probably in error. 18 25.0 -01 35 AC 11 P = 240yr., a = 0.59", motion retrograde in a highly- inclined orbit. Spectrum composite; A9III+F6III. 18 25.3 +48 46 HU 66 Single 1943, 1945 (Van Biesbroeck, 82-inch). 18 25.4 -16 31 HU 64 Mt. Wilson spectral classes F5s and G0. 18 25.4 -20 33 JC 6 21 Sgr. 18 25.5 -66 05 HJ 5039 B is CPD-66@3337. 18 25.9 +60 29 ES 2666 Proper motion of B -007 -018. 18 26.2 +08 47 LDS 1012 B is BD+08@3692. 18 26.4 +46 49 STT 352 B is BD+46@2489. Proper motion of B -020 +016. 18 26.6 +06 32 SCJ 17 Proper motion of B +009 +004. 18 26.7 +26 27 BU 1326 A is a spectroscopic binary. 18 26.9 +40 31 ES 1653 Proper motion of B +009 -032. 18 27.2 +00 12 STF 2316 59 Ser. A is a triple spectroscopic binary, and B may be a spectroscopic binary also. A is an irregular variable, d Ser. 18 27.5 -15 22 J 1631 CD is probably AB of 18275-1524 with quadrant reversed. 18 27.7 -32 07 I 1023 Measures uncertain, too close. Duplicity dubious, but needs speckle. 18 28.0 +06 12 CHR 71 P = 11.12yr., a = 0.12", motion retrograde. 18 28.4 -15 27 FOX 82 May be component of multiple 18275-1524. 18 28.6 +04 51 STT 168 B is BD+04@3759. Proper motion of B +008 +018. 18 28.9 -25 03 H 125 H N 125. 18 29.0 -26 35 WNO 6 Variable? B is CD-26@13205. 18 29.3 -34 31 B 1364 CPD-34@7858. 18 29.5 +29 59 KU 118 Proper motion of B +000 -011. 18 30.0 +01 11 STF 2321 Proper motion of B -006 -004. 18 30.0 -12 57 HU 69 Spectrum: B9.5II/III. 18 30.1 +04 04 STF 2322 Proper motion of B -013 +006. 18 30.3 +32 46 SLE 184 Proper motion of B -004 +018. 18 30.7 +04 31 STT 170 B is BD+04@3775. Proper motion of B -011 -014. 18 30.9 +38 40 STF 2338 C is the semiregular variable KP Lyr. Proper motion of B -022 +023. 18 30.9 -14 56 FOX 231 Proper motion of B -007 000. 18 31.2 +66 08 ES 1911 Proper motion of B +016 +004. 18 31.2 +65 26 KUI 86 A is a spectroscopic binary. 18 31.2 +13 11 STF 2330 B is BD+13@3668. Proper motion of B +010 -001. 18 31.3 -55 32 HJ 5044 B is CPD-55@8709. 18 31.4 -43 22 CPO 81 Proper motion of B -065 -215. 18 31.7 +23 10 HU 321 Mt. Wilson spectral type of B is G0. 18 31.9 -19 08 BU 966 Cluster M 25. A is the Cepheid U Sgr. Identifications on Hyd. ph. -19@, 18:28 are as follows: A 51273 G 51291 P 51300 B 51272 H 51271 Q 51299 C 51297 J 51270 R 51274 D 51298 K 51267 S 51263 E 51266 L 51268 T 51292 F 51265 M 51269 U Close comp. to B. 18 32.6 -49 36 RST 2060 RST 2060a. 18 32.8 +13 49 STF 2336 Proper motion of B -010 +021. 18 32.9 +38 50 STT 171 B is BD+38@3211. Proper motion of B +110 +080. 18 33.1 -19 18 J 2215 CPD-19@6927. 18 33.4 -38 44 DUN 222 Kappa (2) Cra. B is CD-38@12896, Kappa (1) Cra. Proper motion of B +001 -024. 18 33.5 +07 26 SCJ 18 B is BD+07@3740. Proper motion of B -015 +010. 18 33.8 +70 03 STF 2370 Proper motion of B +074 000. 18 33.8 +17 44 HU 322 Distance less than 0.1" in 1960. 18 33.9 +52 21 A 1377 P = 191yr., a = 0.26", motion direct. C is physical. Proper motion of C -023 -009. Mt. Wilson spectral classes A is G5, C is B8n. 18 34.5 -37 53 JSP 780 CPD-37@8199. 18 34.6 -27 34 I 1027 CPD-27@6461. 18 34.7 -65 57 I 634 Spectrum: G3/6III+(A). 18 34.9 -14 42 STF 2337 B is BD-14@5117. Proper motion of B +011 -016, spectrum: B9/A0II/III. 18 34.9 -48 01 HJ 5047 B is CD-48@12597. 18 35.0 +11 27 STF 2341 Proper motion of B -005 -007. 18 35.4 +06 49 J 100 Van Biesbroeck calls this Toulouse +7@, 18h 28m No. 300. Jonckheere gives BD+06@3866. 18 35.5 +23 36 STT 359 P = 211yr., a = 0.42", motion retrograde. Spectrum composite; G9III+G7III. 18 35.5 +21 04 STF 2345 Proper motion of B -013 +001. 18 35.6 +04 56 BU 643 A is the Alpha CVn-type variable FR Ser. 18 35.9 +16 59 STT 358 P = 380yr., a = 1.84", motion retrograde. Alternative spectrum: G2V+G2V. 18 36.0 +11 44 STT 357 P = 324yr., a = 0.46", motion retrograde. 18 36.1 +64 05 MLB 214 Position corrected by Heintz. 18 36.2 +41 17 STF 2351 Proper motion of B +007 +013. 18 36.4 -49 52 CPO 592 CPD-49@10659. 18 36.5 -11 59 BAR 10 Round in 1958, 1961. No positive measures since 1952. 18 36.6 +33 28 STF 2349 A is possibly a spectroscopic binary. Variable. 18 36.7 +06 40 CHR 76 A is a spectroscopic binary, now resolved by speckle. 18 36.8 +21 20 HU 323 Too close in 1958 (82-inch). 18 36.8 +11 51 L 39 The Sternberg measure evidently does not belong to this pair. 18 36.8 -26 17 RST 3187 Too close in 1959, 1962. 18 36.9 +38 46 H 39 AB: H V 39. Alpha Lyr. Proper motion of B +004 -006. Proper motion of B +002 +013. STF 9 AE: Proper motion of E +007 -004. The components are optical. 18 37.3 +07 32 STF 2346 B is BD+07@3773. Proper motion of B -008 +001. Optical. 18 37.4 +77 41 STT 363 P = 309yr., a = 0.34", motion direct. 18 37.5 -68 56 LDS 643 Separation 1065". 18 37.9 +28 23 AG 362 Proper motion of B -022 -010. 18 38.4 +67 08 STF 2384 P = 133.5yr., a = 0.615", motion direct in a highly- inclined orbit. 18 38.4 +63 32 STF 2377 Proper motion of B -026 +010. 18 38.4 +08 50 HU 198 X Oph, a Mira-type variable. A premature orbit has been computed. However, the apparent motion is nearly rectilinear. Spectrum composite; K1III+M6IIIe. 18 38.4 -03 12 A 88 P = 12.1yr., a = 0.148", motion retrograde. 18 38.6 +16 32 HO 87 P = 124yr., a = 0.28", motion direct. 18 38.7 +28 47 L 25 L 25a. 18 38.7 +24 39 HJ 1332 B is BD+24@3479. 18 38.9 +52 21 STF 2368 Mt. Wilson spectral classes A1n and G0. Proper motion of B +011 -001. 18 40.1 +03 21 AG 224 Proper motion of B +006 -003. 18 40.4 +09 42 S 704 B is BD+09@3814. Proper motion of B -004 -014. 18 40.6 +03 07 STF 2361 B is BD+02@3649. Proper motion of B +035 -029. 18 40.8 +12 14 HJ 1334 Probably same as J 2142. J gives BD as +12@3414; perhaps misprint for BD+12@3614. 18 40.9 +31 32 HJ 1337 Proper motion of B +038 -850. 18 41.0 +24 50 A 2988 P = 52yr., a = 0.17", motion retrograde. 18 41.3 +30 18 STF 2367 P = 93yr., a = 0.26", motion retrograde. Proper motion of B +025 -060. C is physical. Bidelman classifies AB as composite gK+A:. 18 41.8 +33 14 KU 119 Proper motion of B +028 +006. 18 42.1 +34 45 B 2546 A is called a spectroscopic binary, but the variation is likely caused by motion in the close visual pair. B is BD+34@3286. Proper motion of B +025 +010. 18 42.2 +27 39 STF 2371 Proper motion of B -009 -007. 18 42.2 -10 22 J 2522 J 1655 is probably identical. 18 42.3 -09 03 RST 4594 Delta Scuti, prototype of the Delta Scuti variables. H 36 AC: H V 36. 18 42.6 +55 32 ISO 7 46 Dra. A spectroscopic binary, P 9.87d. Abundance peculiarities. 18 42.6 -47 40 HJ 5054 B is CD-47@12469. 18 42.7 -23 36 BRT 1542 Proper motion of B +038 -023. 18 42.8 +59 38 LDS 1466 Proper motion of B -1315 +1815. 18 42.9 +44 56 STF 2380 B is BD+44@2974. Proper motion of B -001 -013. 18 43.0 -71 26 HJ 5048 Zeta Pav. 18 43.1 +07 42 LDS 1013 B is BD+07@3814. 18 43.2 +59 33 STF 2398 P = 408yr., a = 13.88", motion direct. AB: Mt. Wilson spectral classes of A and B M4. Proper motion -1298 +1879. B is variable. AC: Same as ADS 11632 AB. 18 43.3 +39 18 BLL 35 A spectroscopic binary. B is BD+39@3504. 18 43.3 +25 06 COU 509 POU 3503 identical? 18 43.4 +35 33 STF 2378 Proper motion of B +005 +005. 18 43.4 -55 46 B 398 P = 48yr., a = 0.27", motion retrograde. 18 43.5 -08 17 J 104 Epsilon Scl. 18 43.6 -51 38 RST 5451 A is variable. Spectral type A2/3III/IV. 18 43.7 +31 41 A 253 P = 99yr., a = 0.47", motion direct. 18 43.7 +30 24 STF 2376 Proper motion of B +006 +019. 18 43.7 +05 39 STT 361 Proper motion of B +010 +008. 18 43.8 -38 19 COO 227 11 Cra. Variable? 18 44.3 +39 40 STF 2382 Epsilon (1) Lyr. 4 Lyr. AB: A premature orbit has been computed. STF 37 AB-CD: STF 37. See ADS for notes of components. STF 2383 Cc-D: Epsilon (2) Lyr. 5 Lyr. P = 724yr., a = 2.92", motion retrograde. C is an Alpha CVn-type variable, and has a companion, c. 18 44.5 +34 00 STT 172 B is BD+33@3191. Proper motion of B +006 -020. 18 44.8 +37 36 BU 968 Zeta (1) Lyr. A is a spectroscopic binary and variable. STF 38 Zeta (2) Lyr. 18 44.8 -34 49 BRT 1786 CPD-34@8050. 18 44.9 +16 06 HEI 173 A third star at 323 degrees, 62". 18 45.2 +39 14 STF 2392 Proper motion of B -007 -028. 18 45.2 +35 32 STF 2386 B is BD+35@3350. Proper motion of B +007 -019. 18 45.4 -50 25 R 313 B is CD-50@12120. 18 45.5 +05 30 FIN 332 A remarkable quadruple system. 18 45.7 +20 33 HJ 2839 110 Her. 18 46.2 +64 12 HU 937 P = 303yr., a = 0.61", motion direct. 18 46.3 -22 24 SEE 360 28 Sgr. 18 46.3 -27 21 B 405 P = 105yr., a = 0.40", motion retrograde. 18 46.4 -35 59 BRT 1787 CPD-36@8476. 18 46.5 -00 58 MCA 53 Aa: 5 Aql. A suspected spectroscopic binary, now resolved by speckle interferometry. 18 46.6 +38 21 HU 1191 P = 14.7yr., a = 0.21", motion retrograde. 18 46.9 -12 22 BRT 2757 Possibly BD-12@5164. J 2147. 18 47.0 +18 11 ENG 64 111 Her. 18 47.3 +28 25 HJ 1347 Proper motion of B +007 +021. 18 47.4 -21 08 B 1889 Spectrum: B9.5II/III. 18 47.5 +49 26 BU 971 The primary is a spectroscopic binary, and is also the semiregular variable S Sct. 18 47.7 +36 00 ALI 142 A is the RR Lyrae-type variable EZ Lyr. 18 47.9 +11 10 STT 174 B is BD+10@3660. Proper motion of B +010 +005. 18 48.3 -20 33 DON 924 CPD-20@7194. 18 48.7 -17 02 J 2235 Spectrum: G6/8III/IV. 18 48.9 +16 15 STF 2400 AC: Mt. Wilson spectra are F5s for A and A4n for C. AD: D not seen in 1901 and 1919. 18 49.6 +38 18 AG 226 Proper motion of B +012 -028. 18 49.6 +10 48 GAN 6 This may be STF 2408, BDS 8876. 18 49.7 -05 55 H 50 H VI 50. C is BD-06@4923. Proper motion of C +001 +008. A is a long-period spectroscopic binary. 18 49.7 -20 19 SEE 362 29 Sgr. Spectroscopic binary. 18 49.7 -73 00 R 314 A is a spectroscopic binary. 18 49.8 +32 49 H 40 H V 40. Nu (1) Lyr. A is a Beta Lyrae-type system. 18 49.9 +32 33 HO 440 Nu (2) Lyr. 18 50.0 +20 43 HU 328 A is the Algol-type system AD Her. 18 50.1 +33 22 STF 39 Beta Lyrae. A is the prototype variable of its class. B is BD+33@3224. Proper motion of B -014 -013. 18 50.3 -07 54 BU 969 S Scuti, variable 9.7-10.9, 148 days. 18 50.8 +10 59 STF 2404 A spectroscopic binary. Composite spectrum, K5III+K3III. 18 50.8 -22 10 BU 1300 30 Sgr. 18 50.9 +11 06 COU 16 May be same as BRT 1312 at 18 50.9 +11 09. 18 51.2 +59 23 STF 2420 Omicron Dra. A is a spectroscopic binary. Proper motion of B -016 +020. A is also variable. 18 51.2 -00 37 A 860 Too close 1954-1984. 18 51.8 -21 41 DON 929 CPD-21@7088. 18 51.9 -57 56 HJ 5065 B is CPD-58@7511. Proper motion of B -006 -039. 18 52.1 +24 31 COU 510 One component is an Algol-type system, JZ Her. 18 52.2 -62 11 HJ 5062 Lambda Pav. A is a Cepheid. 18 52.3 +39 26 WEI 33 B is BD+39@3557. Proper motion of B -009 -018. 18 52.3 +21 26 ISO 8 112 Her. A spectroscopic binary, P = 6.36d. The inter- ferometer pair cannot be this object, so the system is triple. 18 52.3 +14 32 STF 2411 Proper motion of B -001 -029, spectrum F7V. It is called a spectroscopic binary. 18 52.8 +31 25 A 257 Also a faint unequal pair about 28" from CD in 226@. 18 52.8 +12 34 AG 365 B is BD+12@3695. 18 52.8 -17 25 HU 257 Spectrum: Fm Delta Del. 18 53.0 +36 21 HJ 1354 Proper motion of B +017 -020. 18 53.4 +03 23 STF 2413 Proper motion of B +004 -051. 18 53.5 +75 47 STF 2452 A spectroscopic binary. 18 53.5 -20 30 DON 933 CPD-20@7296. 18 53.6 -19 41 RST 3203 Spectrum: A2/3II/III. 18 53.7 +36 58 H 3 H VI 3. Delta (1) Lyr. A is a spectroscopic binary. B is BD+36@3308. 18 53.7 -05 33 A 93 P = 239yr., a = 0.55", motion direct. 18 54.2 -22 45 BU 1033 Nu (1) Sgr. 18 54.5 +36 54 ES 2028 Delta (2) Lyr. A is an unclassified variable. 18 54.6 +27 54 BRT 3335 ADS 11819a. 18 54.7 +22 39 BU 646 113 Her. The G-type component is a long-period spectroscopic binary. 18 54.9 +33 58 STT 525 A is a spectroscopic binary. C is BD+33@3256. 18 54.9 +08 30 HU 259 Distance < 0.1" 1954-1960 with 82-inch. 18 55.3 -23 41 B 412 Spectrum: B9.5III/IV. 18 55.3 -26 18 SMY 4 Sigma Sgr. B is CD-26@13591. 18 55.4 +13 31 BU 647 Also Duner 2, BDS 8899. Identification and position correction by Heintz. 18 55.8 +03 27 A 2192 P = 132yr., a = 0.28", motion retrograde. 18 55.9 +03 23 A 2193 Quadrants uncertain. 18 56.0 +44 14 STT 365 AB: Duplicity doubtful, needs speckle. STF 3130 Lewis measures a pair 1m following and 1' south: 1897, 37@, 3.1", 10.0-11.0. 18 56.0 +33 47 STF 2421 B is BD+33@3264. 18 56.2 +04 12 STF 2417 Theta (1) Ser. B is BD+04@3917, Theta (2) Ser. 18 56.2 -50 49 RST 1011 Spectral type G8/K0 II/III. 18 56.4 +45 30 HJ 1356 B is BD+45@2796. Proper motion of B +020 +064. 18 56.4 -40 40 WG 238 CPD-40@8697. 18 56.9 +31 12 ES 2422 A is the irregular variable OQ Lyr. 18 56.9 +15 46 L 42 Baize questions BD identification. Heintz and Worley cannot locate this pair. Identical to OL 180? 18 56.9 -33 20 GLP 15 B is CD-33@13738. Proper motion of B +035 +022. 18 57.0 +32 54 BU 648 P = 61.2yr., a = 1.26", motion retrograde. 18 57.3 +62 24 STF 2440 Spectrum of A also called composite; G5IV+G8V. Proper motion of B +001 -053. 18 57.4 +21 29 HU 329 Many negative results, but probably double. 18 57.5 +58 14 STF 2438 P = 259yr., a = 0.60", motion retrograde. 18 57.7 +15 09 OL 180 Position and Durchmusterung correction by Heintz. 18 57.7 +09 42 HJ 5505 B is BD+09@3942. Proper motion of B +019 -023. 18 57.8 -38 02 B 414 Spectral type K? 18 57.9 -25 24 B 2871 Spectrum: F2/3III/IV. 18 58.1 +38 13 STF 2427 B is BD+38@3377. 18 58.1 +05 59 OL 215 Proper motion of B -006 +007. 18 58.2 +17 22 CHR 82 Aa is the Cepheid FF Aql. The system is also a long- period spectroscopic binary, now resolved by speckle. 18 58.2 -20 25 HO 271 A is a double-lined spectroscopic binary. 18 58.8 +40 41 STF 2431 BDS 8981, H IV 93 is identical. A spectroscopic binary. 18 58.9 +32 41 AGC 9 Gamma Lyr. Variable? 18 59.0 -01 39 BAL 588 Proper motion of B -009 -009. 18 59.1 +13 38 STF 2424 11 Aql. Proper motion of B +009 -012. 18 59.4 -12 50 KUI 89 A light variable. P = 92yr., a = 0.24", motion direct. 18 59.5 +43 44 A 588 A 4" pair of 15th magnitude is 20" south of AB (Burnham). 18 59.6 +15 04 ENG 65 Epsilon Aql. A is a spectroscopic binary. Spectral type K1IIICN0.5Ba0.2. 18 59.9 +14 54 STF 2428 Proper motion of B +013 -008. 19 00.0 +12 53 STF 2426 Proper motion of B -011 +009. 19 00.6 -08 07 STF 2425 B is BD-08@4810. Proper motion of B -003 -011. 19 00.8 -00 27 HJ 874 Bloch measures 1923.7, 260@, 16.96", which may belong to STF 2426. 19 01.1 -36 57 JOY 7 A is the T-Tauri variable S CrA. 19 01.1 -37 04 BSO 14 B is CD-37@13017. Both components are spectroscopic binaries. Proper motion of B +008 -014. 19 01.2 +12 53 J 1279 Not found in 1959 by Van Biesbroeck. He suggests it may be ADS 12017. Found by Heintz, who notes that the OL pair at 19 02.6 +12 56, is identical. 19 01.4 +46 56 HJ 1362 16 Lyr. 19 01.4 -35 48 BRT 1794 CPD-35@8339. 19 01.6 -36 53 B 957 A is the irregular variable TY CrA. 19 01.9 -36 20 B 958 Spectral type M? 19 02.0 +08 46 BU 973 Van Biesbroeck notes that this group is misidentified in both BDS and ADS as BD+08@3945 rather than the correct BD+08@3948. The latter is already identified with ADS 11954, J 533. It seems advisable to keep the ADS number 11947. Here AB is BU 973, STF 2435 = AC of J 533. AD = AB of J 533. DC = Howe 45 is BC of J 533. Proper motion of B +033 +006. 19 02.1 +52 16 STF 2450 A is physical, and shows slow retrograde motion. HU 757 BC: P = 138yr., a = 0.20", motion retrograde. 19 02.1 +02 30 BAL 1973 Proper motion of B -001 -010. 19 02.2 +08 45 STF 2436 B is BD+08@3949. Proper motion of B +033 +006. 19 02.6 -29 53 HDO 150 Zeta Sgr. AB: P = 21.1yr., a = 0.53", motion retrograde. Spectrum composite; A2III+A4IV. H 78 AB-C: H V 78. 19 02.7 -00 43 STF 2434 BC: P = 292yr., a = 1.53", motion retrograde. 19 02.8 +31 23 STF 2441 BDS 9008; H I 60 is probably same star. Proper motion of B: +004 -006. 19 02.9 -03 42 A 3105 14 Aql. Rapidly moving binary, position angles scattered. 19 03.5 -68 45 FIN 357 P = 14.4yr., a = 0.16", motion retrograde. 19 03.7 +57 27 ARG 33 A is the Algol-type system BH Dra. Proper motion of B -017 -007. 19 03.7 +16 58 STF 2442 Proper motion of B +001 -001. 19 03.7 -22 43 DON 945 A is the semiregular variable SU Sgr. 19 03.8 +12 34 J 534 Proper motion of B +012 +004. 19 03.9 +34 09 BU 1285 A: Burnham noted "possibly a close pair". Aitken found it single in 1899. 19 03.9 +26 42 A 2992 P = 87yr., a = 0.17", motion retrograde. Possibly ambiguous. 19 04.0 -38 04 I 1391 P = 46.4yr., a = 0.20", motion direct. 19 04.1 +14 47 STF 2443 Proper motion of B +006 +015. 19 04.2 -22 54 H 129 H N 129. 19 04.3 -21 32 H 126 H N 126. P = 356yr., a = 1.37", motion retrograde. 19 04.6 +23 20 STF 2445 Proper motion of B +018 -001. 19 04.7 -21 44 SEE 369 Omicron Sgr. 19 05.0 -04 02 SHJ 286 15 Aql. B is BD-04@4683. Proper motion of B +034 -036. 19 05.4 +13 52 BU 287 Zeta Aql. A is a spectroscopic binary. 19 05.5 +33 52 HU 940 P = 92yr., a = 0.34", motion retrograde. 19 05.6 -53 47 HJ 5081 B is CPD-53@9461. 19 05.7 +65 02 ES 1914 Position corrected by Heintz, who also notes that the pair J 1353 is identical. 19 05.7 -15 40 HJ 5507 A is a spectroscopic binary. Variable? 19 05.8 +59 18 MLR 217 AB is STI 873, not in WDS because of questionable duplicity. 19 05.8 +38 31 STF 2456 B is BD+38@3428. Proper motion of B -075 -062. 19 05.8 +06 33 STF 2446 Mt. Wilson spectral types F3s and G5. Proper motion of B +019 -087. 19 05.9 +30 04 L 27 Possibly BD+29@3478 (9.3). 19 06.0 +45 49 STF 2463 AC: In Cin. 5 a faint pair is noted: 1879.5, 300@, 18.4". See BDS part II for a discussion of possible identifications. 19 06.0 +35 53 H 103 H V 103. Proper motion of B -010 -020. 19 06.2 +30 26 STF 2454 A premature orbit has been computed for AB. Component A reported double by Dommanget, but observation unconfirmed by observers with larger instruments. However, A is a double-lined spectroscopic binary, P = 27.25d. 19 06.4 +08 14 BLL 36 A is the Mira-type variable R Aql. Proper motion of B -007 -009. 19 06.4 +07 09 STF 2449 Proper motion of B +042 +039. 19 06.4 -10 43 HJ 5090 Proper motion of B -049 -028. 19 06.4 -37 04 HJ 5084 Gamma Cra. P = 122yr., a = 1.90", motion retrograde. 19 06.6 -01 21 STF 2447 Spectrum of B: A0VpSrCrSi. Proper motion of B +007 -020. 19 06.9 +41 37 COU 2197 Measures scattered and impossible to interpret. 19 06.9 +22 10 STF 2455 Mt. Wilson spectral types F1s and B5. 19 06.9 +08 47 HJ 2854 Proper motion of B +012 +030. 19 07.0 +11 04 HEI 568 18 Aql. This is the eclipsing and spectroscopic binary Y Aql, P = 1.30d. He