08001-0937 J  2862     RST 3562.                                                                       
08003+1138 HJ   74     aka ROE  32. Friedrich Damm commented on the declination sign being             
                       wrong for the HJ pair. The 1825 coordinates, precessed to 2000                  
                       match this pair, as does the second measure by John Herschel.                   
08005+2900 OSO  20     G090-036. Common proper motion pair                                     Oso2004 
08005+0955 A  2954     Magnitude underestimated by Aitken; should be ~0.7 mag.                 Baz1951a
08007+1635 BPM 431     [PM2000]  843821 + [PM2000]  843697.                                    Gvr2010 
08009+4452 ES 1325     aka 08017+4451TDS5455.                                                          
08009-0405 LDS6211     NLTT 18799/18798                                                        Chm2004 
08014-5431 DUN  60     One component is variable and a spectroscopic binary.                           
                       dRA = 1.83s.                                                            Dun1829 
08016-3430 JSP 216     CPD-34@1901.                                                                    
08017+6019 MCA  33     53 Cam. A variable of the Alpha CVn type, AX Cam, and a spectroscopic           
                       binary now resolved by interferometry.                                          
                       Value of omega in Baize (1993) orbit incorrectly listed as 113.0, same  Baz1993b
                       as Omega (erratum noted in Inf. Circ. 121, 1994).                       Baz1993d
                       Combined spectroscopic/interferometric orbit by Balega et al. (2004),   Bag2004b
                       yielding mass sum 3.61 +/- 0.38 Msun. Spectral types are estimated as           
                       A2V and F0V.                                                                    
                       Combined spectroscopic/interferometric orbit by Carrier et al. (2002),  CrF2002 
                       yielding a = 275.1 x 10^6 km, parallax 10.2 +/- 1.0 mas and mass sum            
                       1.49 +/- 0.66 Msun. Authors note that Scholz & Lehmann (1988)           Slz1988 
                       attempted to scale their spectroscopic solution using then-available            
                       speckle data, deriving masses for the components of 2.5 and 1.6 Msun,           
                       considerably larger than found here.                                            
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 3.62 +/- 3.60, 3.94, and 2.09 Msun, respectively.             Mlk2012 
08017+2505 H 6  75     ome 2 Cnc = 4 Cnc.  H VI 75.                                                    
08017+1521 BPM 432     [PM2000]  845760 + [PM2000]  845621.                                    Gvr2010 
08017-0836 A  1580     A is the Algol-type system V635 Mon.                                            
08018-3429 I   187     CD-34 4230, mag 11.7, is 46.5" S and a 13.0 is 20" preceding.           Daw1927a
08021+5437 STF1165     Same as STF1166.                                                                
08021-0049 BAL 845     J 3285.                                                                         
08021-1710 HDS1140     AB + TOK 394AC: This is the high-PM M-dwarf LP 784-12 (HIP 39293) at            
                       30pc. A new distant component C was found at 1".8 in addition to the            
                       known pair HDS 1140 which closed from 0".4 in 1991.25 to 0".33 now. It          
                       is confirmed as physical by its fixed position during one year, the             
                       quadrant of the triple was determined in run 5.                         Tok2015c
08024+0409 STF1175     A premature orbit has been computed. Data appear equally well fit by            
                       rectilinear solution - see linear elements catalog.                             
08024+0320 LDS5160     LDS5196.                                                                        
08025+6305 SHJ  86     STTA 90. B is BD+63@750.                                                        
08025-4440 I     8     QQ Pup.                                                                         
08025-5502 HJ 4044     B is CPD-54@1480.                                                               
08026+2028 DOO  47     Doolittle identifies this as BDS 4392, HJ 437 but it seems to be a      Doo1915b
                       different pair.                                                                 
08026+1309 SLE 320     CD: SLE 456.                                                                    
08027-2632 LDS 200     NLTT 18855/18856                                                        Chm2004 
08027-4119 HJ 4038     A component variable? B is CD-40@3775.                                          
08029+0419 BRT2140     BAL 2801.                                                                       
08030-5720 SWR  38     CD-56@ 2090.                                                                    
08031+1637 BPM 433     [PM2000]  848557 + [PM2000]  848413.                                    Gvr2010 
08031-0625 A  1581     A premature orbit has been computed.                                            
08031-3228 HJ 4035     B is CD-32@4768.                                                                
08032-3812 HJ 4039     V626 Pup, EA per 1.425902 d.                                            Zas2011 
08033+5251 HDS1149     An additional component at a distance of 40 mas from the secondary is           
                       suspected in the system. The magnitude difference is between 1.5 and            
                       2 mag.                                                                  Bag2004 
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.42 +/- 0.46, 1.07, and 1.00 Msun, respectively.             Mlk2012 
08035+2748 ES 2628     chi Gem. See Espin.                                                     Es_1908a
08035+1211 HO  350     A=SB?  AB is seen in the 2MASS J,K-band images, but A seems saturated.  Tok2014d
08036-4000 zet Pup     = Naos. The distance estimate is from Reid & Howarth (1996 A&A 311,             
                       616). Van Rensbergen et al. (1996 A&A 305, 825)  discuss the star's             
                       trajectory and possible runaway status.                                 Msn1998a
08037-4634 HJ 4043     B is CD-46@3727.                                                                
08038-1055 J  2492     J 2863.                                                                         
08039-3133 LDS 201     AB: B is CD-31@5466.                                                            
                       AB: SHY 520. Bayesian analysis by Shaya & Olling (2011) indicates very  Shy2011 
                       high (near 100%) probability pair is physical.                                  
                       AC: C is CPD-31@2104.                                                           
           B  2164     CD: TDS5491.                                                                    
08040-5822 BRT3117     TDS5496.                                                                        
08041+3302 STT 187     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.79 +/- 1.42, 4.53, and 2.14 Msun, respectively.             Mlk2012 
08044+1217 BU  581     See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 1.96 +/- 0.38, 1.75, and 0.85 Msun, respectively.  Mlk2012 
                       Star C (mag. 10.5, 5") is in slow direct motion about AB.                       
                       AB,C: Additional notes may be found in Burnham (1894).                  Bu_1894 
08047+2831 MLB 565     Faint pair, 32s p, 3' n of ADS 6557.                                    Baz1951a
                       Probably BRT1937. Barton coordinates agree; measure (165deg, 1.7")              
                       appears reasonable in position angle (with quadrant flip), but with             
                       possible typo in rho.                                                   Brt1936b
08047-6250 DUN  62     A is the variable V375 Car.                                                     
                       B is CPD-62@952.                                                                
08049-0223 GWP 968     ABL 181.                                                                Tob2012b
08052-4525 JC   12     B is CD-45@3742.                                                                
08053-4626 CPO 192     TDS5515.                                                                        
08055-6952 HJ 4055     SWR  39. CPM pair                                                       Skf2004 
08056+2830 MLB 566     The Barton pair formerly at 08049 is identical                          Hei1985a
08056+2732 STF1177     17 Cnc                                                                          
08056-6617 GLI  81     B is CPD-65@867.                                                                
08057+6823 STF1164     Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
08059-2014 ALD  84     CPD-19@3088.                                                                    
08061-0047 A  1971     A premature orbit has been computed.                                    Cou1953d
08062+0201 J   420     Appears to be in rapid retrograde motion.                                       
08063-4021 RSS   9     This previously uncataloged double star was a Hipparcos double entry            
                       system.  The first measure is determined from the individual positions          
                       listed by Rousseau et al.                                               Rss1996 
08068+3303 AG  147     SEI 487.                                                                Nsn2017b
08068-0900 GWP 972     ABL 182.                                                                Tob2012b
08069-1320 GWP 973     ABL 183.                                                                Tob2012b
08069-2707 DUN  61     B is CD-26@5531.                                                                
08069-6618 LUH   5     Primary is the DQ white dwarf WD 0806-661 = GJ 3483, mass 0.62 +/-              
                       0.03 Msun. Mass of companion estimated at ~7 Mjup, Teff ~300K.          Luh2011 
                       Companion Teff 300-345K, mass 6-9 Mjup, distance 19.2 +/- 0.6 pc.       Luh2012 
08071-2138 B  2168     CPD-21@3163.                                                                    
08072+1615 BPM 434     [PM2000]  856195 + [PM2000]  856322.                                    Gvr2010 
08072+0723 AG  149     HJL  86.                                                                HJL1986 
08075+1318 BPM 435     [PM2000]  856648 + [PM2000]  856681.                                    Gvr2010 
08075-2418 RST5284     rho Pup = 15 Pup = Tureis. A is a Delta Scuti-type variable.                    
08076-0814 GWP 976     ABL 184.                                                                Tob2012b
08079-0215 GWP 977     ABL 185.                                                                Tob2012b
08079-6837 RMK   7     eps Vol. A is a spectroscopic binary.                                           
08081-2415 BRT1448     Aka ARA2099.                                                                    
08082+7155 LDS1667     NLTT 18921/18913                                                        Chm2004 
08082+2106 COU  91     LDS 902.                                                                        
                       NLTT 18979/18980                                                        Chm2004 
08084-0005 GWP 979     ABL 186.                                                                Tob2012b
08085+5130 ES   70     27 Lyn.                                                                         
08086-0259 STF1190     zet Mon = 29 Mon. C is BD-02@2449.                                              
                       AB: H 4  97.                                                            MEv2010 
08087+5750 A  1075     Also known as HDS1161. These two pairs were recognized to be the same           
                       by Brian Skiff.                                                         Skf2004 
08089+2437 NLTT 18995  Ren & Fu (2013) calculated an astrometric orbit, combining Hipparcos            
                       Intermediate Astrometric Data with spectroscopic elements by                    
                       Latham et al. (2002). They derived component masses 0.92 and 0.62 Msun  Lat2002 
                       and an estimated semimajor axis of 25.73 mas.                           Ren2013 
08090+3249 DYR   1     VYS 250. A is a flare star, and B is a double-lined spectroscopic               
                       binary, P = 6.21d.                                                              
08090-6118 EHR  11     Companion appears to be a background star.                              Ehr2010 
08091-3719 BRT1615     CPD-36@1978.                                                                    
08091-3931 GLI  80     B is CD-39@4038.                                                                
08092+1836 SLE 466     BC: Hipparcos suspected non-single.                                             
08094+3752 STF1184     B is BD+38@1869.                                                                
08095+3213 STF1187     Hopmann orbit rejected from Fourth Orbit Catalog                        Hop1971 
                       ("period over 4000 years")                                              Wor1983 
           CHR 190     Aa,Ab: Four observations 1991-1996, with separation decreasing from             
                       0.15" to 0.06"; next observed in 2004 at 0.16". Two possible orbits             
                       are suggested: a short-period (11.3y) solution predicts a separation            
                       of 0.074", while a long-period (28.8y) solution predicts 0.143".        Hrt2009 
08095-4720 DUN  65     A: gam 2 Vel. Spectrum WC8+O7.5e, probably the nearest Wolf Rayet.              
                       B: gam 1 Vel. CD-46@3846. Variable, spectrum B1IV.                              
                       AB: Both components are spectroscopic binaries.                                 
                       The AB pair was formerly known as DUN  64.                                      
           I  1175     DE: DE is I 1175 (= RST 4878) at 08 09.5 -47 25.                                
                       The Hipparcos distance suggests a position in front of the Vel OB2              
                       association (van der Hucht et al. 1997 NewA 2, 245; Schaerer et al.             
                       1997 ApJ 484, L153) at a distance of 258 +41/-31 pc; however, the               
                       Hipparcos distances for the B stars in Vel OB2 (Brandt et al. 1971 ApJ          
                       1623, L99) yield a comparable distance of 317 +/- 42 pc.  This is also          
                       consistent with the distance from the resolution of the binary by               
                       Hanbury Brown et al. (1970) of 350 +/- 50 pc.  Thus, we have chosen to  HBr1970 
                       keep gam 2 Vel as a member of Vel OB2. Classification is from van der           
                       Hucht et al. (1997).  The B component was also observed and appeared            
                       to be single. Classifications of the B, C, and D components are from    Msn1998a
                       Hoffleit & Warren (1991).                                               Hof1991 
           TOK   2     Aa: The primary is a close WR+O binary. Although the pair is                    
                       unresolved, VLTI/AMBER observations on 2004.984 over baselines of               
                       46-85m and wavelength range 1950-2170 nm are fit by a binary model              
                       giving a separation of 3.65 +/- 0.06 mas, position angle 72.7 +/- 8.7           
                       deg, flux ratio 0.62 +/- 0.04 (dm 0.52 +/- 0.07 mag.                    MiF2007 
08098-1658 A  3101     Spectrum: A3/5II/III.                                                           
08099-4911 SYO   3     Aka R    81.                                                                    
08100-4241 CPO 195     CPD-42@2143.                                                                    
08102+5548 SHY 524     AC: HIP  40006 + HIP  40536.                                                    
08102+3527 WSI 100     Provisionally designated WSI9105.                                       Hrt2008 
08102+3347 ANR   1     MLB 1049.                                                                       
08102+2551 BUP 111     B is BD+26@1729.                                                                
08103-0607 GWP 984     ABL 187.                                                                Tob2012b
08104+0020 BAL1133     HJL  87.                                                                HJL1986 
08105+2530 BUP 112     psi Cnc = 14 Cnc.                                                               
                       AC: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
08106-1842 GWP 987     ABL 188.                                                                Tob2012b
08106-2024 ARA1030     Aka BRT1454.                                                            Dam2016b
08107-1348 LDS 204     18 Pup. NLTT 19073/19072                                                Chm2004 
                       AB: Both A and B possible SBs?                                          Tok2014d
08107-1751 GWP 989     ABL 189.                                                                Tob2012b
08110+7955 LDS1668     AB: NLTT 18931/18924                                                    Chm2004 
           OSO  21     G251-054. AD is not a proper motion companion                           Oso2004 
08113+0117 STF1198     B is BD+01@2018.                                                                
08113-1256 BU 1064     19 Pup. Not seen in 1936, 1939                                          B__1951a
08114-4259 HJ 4057     B is CD-42@3976.                                                                
08116+3227 CRJ   2     Aa,Ab: Primary is GJ 9256. Crepp et al. (2012) derive spectral types            
                       G4V and M5, masses 0.85 +0.04/-0.03 and 0.16 +/- 0.02 Msun.             CrJ2012 
           STT 564     AB and AC: Optical pairs, based on study of relative motion of the              
                       components using the method of apparent motion parameters.              Kiy2008 
08116-0014 GWP 993     ABL 190.                                                                Tob2012b
08116-3722 JSP 236     CPD-37@1984.                                                                    
08117-0636 J  2054     LAC.                                                                            
08117-3209 B  2170     According to Brian Skiff, while the WDS has the correct position, this          
                       is not CD-31 5661 (a B giant), but instead is CPD-31 2177 an F/G pair.          
                       Appears to be an IDS error.                                             Skf2003 
08118-0717 GWP 994     ABL 191.                                                                Tob2012b
08118-3521 J  2301     Nova Puppis = PK 252-00.1 = CP Pup.                                     J__1962a
08121-1540 HJ 4050     B is BD-15@2309, spectrum A9/F0V.                                               
08122+1739 STF1196     zet Cnc = Tegmine. Reductions of measures in position angle                     
                       untrustworthy because of confusion among the eithr position angles of           
                       minimum visibility. Distance too great for interferometer measures.     WRH1941a
                       AB: H 1  24.                                                            MEv2010 
                       AB: Additional notes may be found in Burnham (1894),                    Bu_1894 
                       Simonov (1937), and                                                     Smw1937 
                       Muller (1955).                                                          Mlr1955c
                       AB,C: H 3  19.                                                          MEv2010 
                       AB,C: 2-orbit AB,Cc quadruple solution (AB,C in HIP).                   Sod1999 
                       AC: Additional notes may be found in Vyssotsky (1936),                  Vys1936 
                       Simonov (1937), and                                                     Smw1937 
                       Simonov (1951).                                                          Smw1951
                       AB,D: D is BD+18@1870.                                                          
                       The system Cc has been resolved by infrared speckle interferometry.     Mcy1983 
                       Typographical error in the Mason et al. (2006) published elements:      WSI2006b
                       omega = 330.2 +/- 6.7, not 6.7 +/- 1.2.                                         
           zet 1 Cnc B This object was misidentified as HR 3210 by McAlister (1978).           McA1978c
08122-0150 J   421     The note in ADS says that the 1906 measures by Morgan, attributed to    A__1932a
                       HJ 778, may belong to this pair.                                        Mrg1907 
08124-0059 GWP 995     ABL 192.                                                                Tob2012b
08125-1502 GWP 996     ABL 193.                                                                Tob2012b
08125-4616 CHR 143     Aa,Ab: Malkov et al. (2012) derive dynamical, photometric, and                  
                       spectroscopic masses 27.06 +/- 23.28, 9.94, 4.79 Msun, respectively.    Mlk2012 
08129+1044 BPM 436     [PM2000]  865688 + [PM2000]  865603.                                    Gvr2010 
08129-0733 LDS5175     LDS6213.                                                                        
08130+5026 GRV1004     SLW 226.                                                                        
08130-5402 HJ 4065     B is CPD-53@1569.                                                               
08131-3435 EVS  13     Primary is the Cepheid RS Pup.                                          Evs2016a
08132-1227 J  1510     BRT 2703.                                                                       
08132-1354 HU  115     Present parallax value adopted instead of poor HIP-value.               Sod1999 
                       See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.46 +/- 0.62, 1.20, and 0.55 Msun, respectively.             Mlk2012 
08136+1527 CLZ  43     Aka FMR 204.                                                                    
08136-0545 HJ 2435     AB: HDO 117                                                                     
                       AB: H 2  87.                                                            MEv2010 
08136-3144 HDO 201     B is below MS, not CPM (NOMAD, WDS). C is below MS, optical.            Tok2014d
08136-4700 GLI  87     A is variable. B is CD-46@3928.                                                 
08137+0407 ARG  68     A is +04 1934b while B is +04 1934a.                                            
08138-2206 LDS 207     CPD-21@3323.                                                                    
                       NLTT 19163/19166                                                        Chm2004 
08138-3444 I   193     For the 1997.1201 measure a smaller annulus was used in the power               
                       spectrum fit due to the faintness of the source. As a consequence, the          
                       separation and position angle uncertainties may be larger than other            
                       measures.                                                               Hor1997 
08140-3619 DUN  67     Variable, OS Pup. B is CD-35@4360.                                              
                       320 Arg. dRA 1.2s, dDEC 1' 12.3". Four stars forming a parallelogram            
                       (with DUN 68, dRA 3.3s, dDEC 1' 41.0", mags 7,7).                       Dun1829 
08140-4021 HJ 4062     The primary is a long-period spectroscopic binary.                              
           h 2 Pup     Hipparcos astrometric solution adopted some elements from the orbit of  HIP1997d
                       Christie (1936).                                                        Crs1936 
08142+1741 H 6  78     AC: H VI 78.                                                                    
           SKF1627     DE: Primary of 08140+1744 found to be D component of 08142+1741.                
08142-3208 HJ 4059     A is a spectroscopic binary.                                                    
08143-3129 B  1592     Spectrum: A1/2III/IV.                                                           
08147-6616 HJ 4075     SWR  41. CPM pair                                                       Skf2004 
08149-0001 J    72     J  1511.                                                                J__1962a
08149+1058 BPM 437     [PM2000]  868831 + [PM2000]  868623.                                    Gvr2010 
08149-0120 J  2055     +1s, +1.5' from BD-05 1945. Companion variable.                         J__1955 
08153-1126 J  2875     BRT 2704.                                                                       
08155+0202 DOB   9     BAL 1840.                                                                       
08155-3722 HJ 4063     B is CD-36@4387.                                                                
08156+1126 LEP  30     NI   18.                                                                        
08157+0738 STF1209     B is BD+08@2015.                                                                
08158+0550 ADM   3     WSP  51. HTP  30. HAT-P-30. Primary is exoplanet host star.             Adm2013 
08159+5047 STF1199     Opik reverses quadrant.                                                         
08159-3056 BU  454     Spectrum composite; G5-8III+G:.                                                 
08159-6252 HJ 4077     B is CPD-62@987.                                                                
08161+5706 ENG  34     AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
           GIC  79     AD: LDS2568.  AD = G194-017/G194-018.                                           
08161+1942 LDS3781     G040-014. See Allen et al. (2000) for information on metallicity,       AlC2000 
                       age, galactic orbital parameters, etc.                                          
                       NLTT 19210/19207                                                        Chm2004 
08161-2847 HLD  95     Spectrum: A2/3III/IV.                                                           
08165+7930 STF1169     HJL  88.                                                                HJL1986 
                       AB: A is SB1, P=4.884d                                                  Tok2014d
08165+0911 BU 1065     bet Cnc = 17 Cnc. Burnham measured BD+09@1922 and BD+09@1926 with       A__1932a
                       respect to A. A may be variable.                                                
08167+3216 ES  293     SEI 489.                                                                Nsn2017b
08167+0113 OL  179     Aka HEI 344.                                                                    
08166-7914 HJ 4105     SWR  42.                                                                        
08169+5503 LDS3780     BC: SLW 231.                                                                    
08169+3331 SEI 490     None of the components seen on POSS plate; may be flaws on AC Potsdam           
                       plate.                                                                          
           SEI 491     AC. See note to SEI 490.                                                        
08170+5911 STT 565     B is BD+59@1153.                                                                
08170+0001 CHM   5     NLTT 19241 + 19240.                                                             
08172+3515 BRT3250     ALI 120.                                                                        
08173-0522 A   337     Only elements P and T have been amended from the orbit of               Sta1977a
                       Baize (1959).                                                           Baz1959 
08174-1125 BRT2708     J 1513.                                                                         
08175+3623 GRV 756     HJL  89.                                                                HJL1986 
08178+3738 BRT2219     ALI 587. Heintz describes this as identical to PTT  20.                 Hei1985a
08178-1927 LDS 211     = GWP1002 = ABL 194.                                                    Tob2012b
08178-6128 HRG  14     Aka HDS1179.                                                                    
08179+0628 STF1213     BDS 4546, HJ 87 probably same star.                                             
08179-5910 HJ 4084     AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
08180-0022 GAU  11     BAL 850.                                                                        
08182-3722 HJ 4073     A is a spectroscopic binary.                                                    
08183+3859 STF1211     AD: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
08184-0803 GWP1003     AB: ABL 195AB.                                                          Tob2012b
           GWP1004     AC: ABL 195AC.                                                          Tob2012b
08184-2017 HJ 2441     A component is close double of spectral types A5III+G0III,                      
                       C component is also a close double of types A0-2III+K0III               AbH2000 
08185-0616 GWP1006     ABL 196.                                                                Tob2012b
08186-0554 GIC  71     G113-026/G113-027. LDS6214. A 1-hour error in transcribing coordinates          
                       led to an incorrect WDS designation for this system of 07185-0550.              
                       It is assumed that Giclas' original value for theta (28deg) was due to          
                       a math error, so it was corrected to 180-28=152deg.                             
                       NLTT 19298/19299                                                        Chm2004 
08186-4254 CPO 198     CPD-42@2341.                                                                    
08187-2033 RSS 154     CPD-20@3578                                                                     
08187-3407 RST2547     CPD-33@2077.                                                                    
08188+6806 LDS2571     NLTT 19229/19230                                                        Chm2004 
08189-3142 PRO  51     Aka TDS5709.                                                                    
08190-7330 HJ 4095     AC = SWR  44. Brightest two stars in a 1' group.                        Skf2004 
08191+1607 BPM 438     [PM2000]  875251 + [PM2000]  875178.                                    Gvr2010 
08193+6230 OS UMa      Ren & Fu (2013) calculated an astrometric orbit, combining Hipparcos    Ren2013 
                       Intermediate Astrometric Data with spectroscopic elements by                    
                       Carquillat et al. (1983).                                               Crq1983 
08193-0537 TOK 121     HIP 40765. Small PM(A)=(-1,+42). NOMAD: PM(B)=(+66,-16), V(B)=12.83.            
                       B can be optical (crowded field, N*=42).                                Tok2011a
08194-3807 JSP 260     CPD-37@2202.                                                                    
08195+3503 STTA 91     B is BD+35@1801.                                                                
                       AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
08198-7131 BSO  17     A: kap 1 Vol. A is a spectroscopic binary.                                      
                       B: kap 2 Vol                                                                    
08199-2418 B   152     HDO 114.                                                                        
08200-5740 CPO 200     B is CPD-57@1483.                                                               
08201+3834 GIC  80     G111-072/G111-071.                                                              
                       NLTT 19314/19311                                                        Chm2004 
08202-5642 SWR  43     CPM pair                                                                Skf2004 
08206-7729 I   799     the Cha                                                                         
08207-0001 SLW 241     ABL 197. GWP1007.                                                       Tob2012b
08211+6527 SHY 199     HIP  40918 + HIP  40882.                                                        
                       AB: A is SB1, P=17.6y; suspected non-single star in Hipparcos           Tok2014d
08211+4725 STT 190     A,Ca: AB,Ca may be a quadruple system, as the proper motions are in             
                       fair agreement..                                                                
                       AB (mag. 8.6-12.0, 4") is HU 224, 39" distant.                                  
                       AD: D is BD+47@1565.                                                            
           STT 190     AC: HJL  90.                                                            HJL1986 
08211+1552 BPM 439     [PM2000]  878193 + [PM2000]  878305.                                    Gvr2010 
08213+3419 LEP  31     NI   19.                                                                        
           BVD 161     AD: X-ray aRX J0821.3+3418 and 2MASS at 5" from A, is it D?             Tok2014d
08213-0136 STF1216     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 8.24 +/- 5.59, 4.58, and 2.09 Msun, respectively.             Mlk2012 
08214-3545 BRT1623     CPD-35@2261.                                                                    
08214-3629 HJ 4085     A is a spectroscopic binary.                                                    
08217+1717 PAR   1     A is the Mira-type variable V Cnc.                                              
08217+1048 BPM 440     [PM2000]  879031 + [PM2000]  878978.                                    Gvr2010 
08217-5841 LDS 216     LDS5695.                                                                        
08221-7324 HJ 4103     eta Vol                                                                         
08223+1558 BPM 441     [PM2000]  879905 + [PM2000]  879851.                                    Gvr2010 
08223-3458 BRT1625     CPD-34@2328.                                                                    
08225+2638 BUP9115     See note to 08231+2648 BUP 115.                                                 
08225-2942 B  1600     Spectrum: Fm Delta Del.                                                         
08225-4829 I    67     B Vel                                                                           
08225-5931 HDS1190     = eps Car = Avior                                                               
08228-2621 B   767     Many negative or uncertain observations.                                        
08228-5727 BRG  27     Aa,Ab: As noted in Bergfors et al (2010), this is a triple system with  Brg2010 
                       component B outside of 6". Hence, we do not include component B in              
                       Table 4, but we note that at 8.429+/-0.001" separation in 2008.88 and           
                       8.374+/-0.003" in 2010.09, there is statistically significant orbital           
                       motion also for this component.                                         Jnn2012 
08228-7626 HJ 4109     B is CPD-76@515.                                                                
08229-5207 SHY 525     HIP  41081 + HIP  40916.                                                        
08231+2648 BUP 115     The IDS incorrectly associated this pair with BD+28 1598, rather than           
                       +27 1602. As a result, it was initially assumed to be a member of a             
                       quadruple system with two other pairs in the IDS. Eventually all were           
                       assigned the discoverer designation BUP 115 and component designations          
                       AB, AC, and CD. However, the two A components differ in precise                 
                       position by some 12.8 arcminutes. They were later assigned different            
                       WDS designations but discoverer and component designations were not             
                       corrected. The AC and CD pairs have now been assigned the designation           
                       BUP9115, with component designations AB and BC.                                 
08231-4912 DENIS-P...  DENIS-P J082303.1-491201 is an L1.5 dwarf at 20.77 +/- 0.08 pc.                 
                       Observations with FORS2 on the VLT reveal an astrometric companion in           
                       an eccentric orbit with period 246.4 +/- 1.4 days.  Masses of the               
                       primary and secondary are estimated at 78.4 +/- 7.8 and 28.5 +/- 1.9            
                       Mjup for an age of 1 Gyr, or 70.2-82.8 and 26.7-29.4 Mjup for ages              
                       0.6-3 Gyr.                                                              SaJ2013 
                       Sahlmann et al. (2015) refine the orbit of this juvenile binary brown           
                       dwarf, deriving spectral types L1.5 +/- 0.6 and L5.5 +/- 1.1, Teff =            
                       2150 +/- 100 and 1670 +/ 140K, log (Lbol/Lsun) = -3.73 +/- 0.08 and             
                       -4.25 +/- 0.20, masses 0.028-0.063 and 0.018-0.045 Msun (mass ratio             
                       0.64-0.74), delta I = 2.3 +/- 1.2 mag. The distance is 20.7pc, the age          
                       estimated to be in the range 80-500 Myr.                                SaJ2015b
08234-1016 GWP1010     ABL 198.                                                                Tob2012b
08234-1115 J  2878     BRT 2709.                                                                       
08234-2207 BRT1457     CPD-21@3515.                                                                    
08234-2310 BRT1458     CD-22@6089.                                                                     
08234-4248 HJ 4090     B is CD-42@4188.                                                                
08235+1434 LDS1210     NLTT 19425/19426                                                        Chm2004 
08236-1920 GWP1011     ABL 199.                                                                Tob2012b
08237-1150 GWP1012     ABL 200.                                                                Tob2012b
08237-2137 B  2654     J  1517.                                                                Nsn2016 
08237-5519 SHY 526     HIP  41147 + HIP  41579.                                                        
08238+5725 STTA 92     B is BD+57@1136.                                                                
                       AB: HJL  91.                                                            HJL1986 
08239+1038 A  2961     21 Cnc.                                                                         
08242-0150 GWP1014     ABL 201.                                                                Tob2012b
08243+4457 STF1217     LDS 904. B is BD+45@1575.                                                       
                       NLTT 19431/19428                                                        Chm2004 
                       HJL  92.                                                                HJL1986 
08243-0424 GWP1015     ABL 202.                                                                Tob2012b
08244-0432 GWP1016     AC: ABL 203.                                                            Tob2012b
                       08243-0432 and 08244-0431 found to share primary. Systems merged.               
08244-4601 CPO 204     CPD-45@2479.                                                                    
08245-3039 HJ 2446     B is CD-30@6203.                                                                
08246-0109 B  2527     FIN measures 1951-1959 distance less than 0.1".                                 
                       AB pair bound; change in separation and angle consistent with orbital           
                       motion. B component likely M2-M5 dwarf with mass 0.24 +/- 0.01 Msun.            
                       C and D components likely unrelated.                                    Egn2007 
                       AB: Likely a spurious pair. Last measured 1961 and unresolved by SOAR           
                       on 3 occasions 2010–2013.                                               Tok201
                       AB: Tentative resolution by Finsen, 1 speckle measure at 0.040" in              
                       2001.08, unresolved by Hipparcos, 3 non-resolutions by SOAR 2010-2013.          
                       AB can be "ghost".                                                      Tok2014d
           EGN  27     AE: E companion was not detected by RoboAO in 2013.05, below limit.     Tok2014d
08246-0345 CHR 172     Aa,Ab. Abt & Biggs (1972) note variable RV.                             AbH1972 
                       Aa,Ab: Likely a spurious pair. Last measured 1988 and unresolved by             
                       SOAR on 3 occasions 2011–2013.                                          Tok201
           TOK  20     AB: GJ 306. AB has estimated period 23,000y; Close triple?              Tok2006 
                       AB: A is SB, P=1.563d.                                                  Tok2014d
08247+4200 S   565     STTA 93. B is BD+42@1860.                                                       
08247-2849 RST1393     A is an Algol-type system, AW Pup.                                              
08248+2009 STT 191     B is BD+20@2078.                                                                
08249+1214 BPM 442     [PM2000]  883581 + [PM2000]  883518.                                    Gvr2010 
08249-4418 DAW 194     Turner (1979 A&A 76, 350) includes this star in the Vel OB1 group at a          
                       distance of 1.8 kpc. Photometric spectral classifications of the B and          
                       C components are from Lindroos (1985), who also finds a                 Lnd1985 
                       distance of 2.7 kpc.                                                    Msn1998a
08250+6725 LDS2574     B is BD+67@541.                                                                 
08250-4246 CHR 226     Ba,Bb: This close companion to RST4888 has been observed on three               
                       occasions, but has shown little movement over a 1.6-year period. The            
                       1989 measurements of the Rossiter pair were originally published by             
                       McAlister et al. (1990) and Hartkopf et al. (1993). Following           McA1990 
                       discovery of the close pair in the 1990 data, these 1989 data were      Hrt1993 
                       rereduced, resulting in "preconfirmation" of the new component.         Hrt1996b
                       V438 Pup, Algol (EA) type eclipsing binary, P = 4.9350 d.               Zas2011 
                       The new pair was initially given component designations Aa,Ab, but              
                       it was uncertain which component of the Rossiter had been split.                
                       Tokovinin et al. (2015) have determined it was the B component, so the  Tok2015c
                       pair has been changed to Ba,Bb.                                                 
08251-4910 RST 321     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.60 +/- 0.14, 1.77, and 0.85 Msun, respectively.             Mlk2012 
08252-2403 S   568     A is a spectroscopic binary.                                                    
                       B is a K1III and is CD-23@7280.                                                 
08253+1030 BPM 443     [PM2000]  884065 + [PM2000]  884231.                                    Gvr2010 
08254+7607 MLR 547     Aka TDS5815.                                                                    
08254+3723 HU  856     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 7.12 +/- 4.20, 3.34, and 1.20 Msun, respectively.             Mlk2012 
08255-5144 DUN  69     B is CD-51@3003.                                                                
08256-5332 BRT3286     CD-53@2275.                                                                     
08258-4155 RST2553     TDS5818.                                                                        
08259+0734 H 5 109     H V 109. HJ  785.                                                               
08260-4318 DON 249     CPD-42@2480.                                                                    
08263-3904 HJ 4093     AB: A is the Algol-type system NO Pup.                                          
08264-0849 GWP1018     ABL 204.                                                                Tob2012b
08265+2754 S   566     22 Cnc = phi 1 Cnc                                                              
08265-0359 H 6 118     H VI 118. 2 Hya. Possible Delta Scuti-type variable.                            
                       BDS 4606 is the same star.                                                      
08267+2432 STF1224     24 Cnc =  ups Cnc.                                                              
           STF1224     A,BC: H 2  41.                                                          MEv2010 
           A  1746     See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       BC: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 3.54 +/- 0.80, 2.50, and 1.13 Msun, respectively.  Mlk2012 
08267-1910 FEN  14     B. J 2640.                                                                      
08267-3155 PRO  59     CPD-31@2369.                                                                    
08268+2656 STF1223     phi 2 Cnc. Both components suspected of variability.                            
                       H 2  40.                                                                MEv2010 
08268-2252 LDS 219     B is BD-22@2275.                                                                
                       NLTT 19552/19555                                                        Chm2004 
08268-3725 ARU   6     Typo in WDS designation - originally listed as 08228-3725.                      
08270-5242 B  1606     Hipparcos parallax 18.50 +/- 0.44 mas. Dynamical parallax 17.5 mas,             
                       masses 1.61 and 1.28 Msun. The orbit by Finsen (1963) is revised here   Fin1963c
                       using the three available speckle measures, leading to a more accurate          
                       period and to the reduced orbit size. Systematic over-estimation of             
                       the separation by Finsen’s visual interferometry is apparent.           Tok201
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.96 +/- 0.45, 2.61, and 2.27 Msun, respectively.             Mlk2012 
08271+2844 FAR   6     SKF  26. Primary is white dwarf WD 0824+288.                            Far2005b
08271+0331 RUC  21     Primary is FG Hya.                                                              
08276+6235 HJ 3309     B is BD+63@799.                                                                 
08276-2051 B  2179     An eclipsing binary, VV Pyx. Aka B  1100.                                       
08277-0425 A   550     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 3.92 +/- 1.07, 2.89, and 1.45 Msun, respectively.             Mlk2012 
08277-0934 GWP1021     ABL 206.                                                                Tob2012b
08280-0312 GWP1022     ABL 207.                                                                Tob2012b
08280-3507 FIN 314     A spectroscopic binary, probably due to motion in the visual pair.              
                       Primary is XY Pyx, a W Uma type eclipsing binary, period 0.92254d.      Zas2012 
                       Aa,Ab: Malkov et al. (2012) derive dynamical, photometric, and                  
                       spectroscopic masses 10.61 +/- 4.80, 10.39, 6.92 Msun, respectively.    Mlk2012 
08281+3332 STT 193     SEI 499. Incorrectly referred to as STF 193 by Scheiner.                Nsn2017b
08282-3643 EGN   7     Single epoch, but the A and B components are likely unrelated. A and            
                       C are unbound.                                                          Egn2007 
08283+3338 SEI 500     Not found by Heintz at IDS position.                                    Hei1987a
08283-1736 GWP1023     ABL 208.                                                                Tob2012b
08283-4430 RSS 162     AC: Also known as HDS3409AC.                                                    
08285-0231 A   551     A and B are SB's with P = 2.5 d and 6 d, respectively, and star C               
                       (mag. 10.49, 18") appears physical, so that the system is quintuple.            
                       Primary is eclipsing binary LO Hya (period 2.49956 day).                Zas2010 
                       AB,C = STF 1233.                                                                
                       See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       AB: All speckle measures are discordant with the published orbit of     B__1953b
                       van den Bos (1953).                                                     Hrt1992b
08286+6602 JNN 273     Estimated age 300-1000 Myr; masses 0.15 +/- 0.02 and 0.11 +/- 0.01              
                       Msun; a ~4.9 au.                                                        Jnn2014 
08286+5439 MLR 672     Also known as TDS5857.                                                          
08289-4235 HJ 4102     B is CD-42@4287.                                                                
08290+4706 GRV1005     SLW 257.                                                                        
08291+1010 BRT3376     Unnumbered pair, following BRT1250 in Barton's list.                    Brt1935a
08291-1219 GWP1025     ABL 209.                                                                Tob2012b
08291-3456 BRT1630     CPD-34@2548.                                                                    
08291-4756 FIN 315     One component is a spectroscopic binary.                                        
                       Aa,Ab: Docobo & Andrade (2013) derive a dynamical parallax of 3.88 +/-          
                       0.56 mas and component masses 6.08 +/- 3.43 and 5.45 +/- 3.08 Msun              
                       (for spectral type B1.5V) or 3.85 +/- 0.58 mas, 6.27 +/- 3.63 and 5.53          
                       +/- 3.20 Msun (for B2IV). See paper for extensive notes on system.      Doc2013d
08291-6152 TOK 122     HIP 41620. NOMAD: PM(B)=(-21,-3), V(B)=13.21. B is optical based on             
                       the CMDs. PM(A)=(-41,+14).                                              Tok2011a
08295-4443 DUN  70     One component is a spectroscopic binary.                                        
08296+5203 SIN  39     AC: The companion noted by Sinachopoulos & Seggewiss (1990) at (104deg, Sin1990 
                       229") is not seen on Aladin plates. This star at (102deg, 266") agrees          
                       with their magnitude estimate and appears to be the most likely                 
                       candidate for the C component.                                                  
08296-1704 GWP1026     ABL 210.                                                                Tob2012b
08296-3836 I   394     IRAS 08277-3826 = PDS 31.                                               Gre1992 
08299+3123 STF1231     SEI 502.                                                                Nsn2017b
08299-0030 J  1523     BAL 852.                                                                        
08300+2655 ALP  13     2MASSW J0829570+265510                                                          
                       Physical companionship to this ultracool dwarf ruled out based on i-z           
                       and z-J colors, using photometry from SDSS.                             AlP2007 
08301+0412 LDS5696     LDS6216.                                                                        
08303+6253 LDS2282     LDS5197.                                                                        
08303+6043 BU 1067     1 UMa = omi UMa = Muscida. A is variable.                                       
08303+2214 HRO   1     Primary is K2-34, a relatively metal-rich F star. Companion is a hot            
                       Jupiter, mass 1.773 +/- 0.086 Mjup, radius 1.44 +/- 0.16 Rjup           Hro2016 
08303-2602 B   158     ADS 6847a.                                                                      
08305+2818 HJ  788     B component is of spectral type K1III                                   AbH2000 
08306-4031 DUN  71     B is CD-40@4330.                                                                
08307-1610 GWP1027     ABL 211.                                                                Tob2012b
08307-4309 DON 256     CPD-42@2600.                                                                    
08308+1243 BPMA 36     [PM2000]  891033 + [PM2000]  891175.                                    Gvr2010 
08310+4012 SKF 207     For astrometric analysis of 2MASS J08310177+4012115, we compare our             
                       AstraLux measurement with the data from the original discovery as               
                       listed in the WDS. Since there are no error bars quoted, it is                  
                       difficult to formally establish physical companionship. However, even           
                       if we assume that the errors are +/-0.5" and +/-5deg, which should be           
                       very conservative, the background hypothesis can still be firmly                
                       excluded with ~5 sigma confidence. We therefore count it as a                   
                       confirmed companion.                                                    Jnn2012 
08312-1100 GWP1029     ABL 212.                                                                Tob2012b
08313-0601 LDS 221     NLTT 19692/19697                                                        Chm2004 
08313-1938 J  1524     Aravamudan gives position 08267-1916 (1900).                            Ara1963 
08313-8441 HJ 4158     B is CPD-84@192.                                                                
08314+3156 STF1236     B is BD+32@1747.                                                                
                       Additional notes may be found in Lau (1908).                            Lau1908c
08314-3642 LDS 223     C is CPD-36@2622.                                                               
08314-3904 HJ 4107     A is a spectroscopic binary.                                                    
08315-2541 I   805     AC Pyx, Algol (EA) type eclipsing binary, P = 7.66793 d.                Zas2011 
08316+3458 HU  716     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.58 +/- 0.23, 1.77, and 0.95 Msun, respectively.             Mlk2012 
08316+1806 HJ 2452     the Cnc = 31 Cnc. Occultation double.                                           
                       AB: H 5  59.                                                            MEv2010 
08317+1924 LDS 905     AB: NLTT 19685/19684                                                    Chm2004 
                       CU Cnc and CV Cnc. This is a known quintuple system, as reported in,            
                       e.g Delfosse et al. (1999) and Beuzit et al. (2004). Four of the        Del1999a
                       components are resolved in two separate pairs (Aa,Ab and Ba,Bb) by      Beu2004 
                       AstraLux. The fifth component is unresolved in the images; this is an           
                       eclipsing binary companion to the Aa component.                         Jnn2014 
           BEU  12     Aa,Ab: Estimated age 30-300 Myr; masses 0.20 +/- 0.09 and 0.04 +/-              
                       0.03 Msun; a ~6.0 au.                                                   Jnn2014 
           DEL   1     Ba,Bb: Estimated age 30-300 Myr; masses 0.24 +/- 0.12 and 0.18 +/-              
                       0.09 Msun; a ~10.6 au.                                                  Jnn2014 
08317-0619 TOK  21     Additional faint companion seen; not detected in J band, so concluded           
                       was probably optical.                                                   Tok2006 
08318-0347 J   416     C was not seen in 1950                                                  VBs1954 
08319+5037 CRJ   3     Primary is NLTT 19673. Crepp et al. (2012) derive spectral types G1V            
                       and M3-M4, masses 1.04 +0.06/-0.05 and 0.31 +/- 0.03 Msun.              CrJ2012 
08319+3309 STF1238     SEI 503.                                                                Nsn2017b
08319-0300 GWP1032     ABL 213.                                                                Tob2012b
08320+1620 BPM 444     [PM2000]  892430 + [PM2000]  892422.                                    Gvr2010 
08322-1750 GWP1034     ABL 214.                                                                Tob2012b
08323+1520 BPM 445     [PM2000]  892771 + [PM2000]  892635.                                    Gvr2010 
08323-7656 TOK 123     HIP 41871. Astrometric binary in Hipparcos.                                     
08324-0056 HJ   96     B is BD-00@2012.                                                                
                       AB: HJL  94.                                                            HJL1986 
                       AB: SHY 527. Bayesian analysis by Shaya & Olling (2011) indicates very  Shy2011 
                       high (near 100%) probability pair is physical.                                  
08326+0829 STF3119     Also known as STF3066.                                                          
08326-1502 B  2528     Likely a spurious pair. Last measured 1942 and unresolved by SOAR on 4          
                       occasions 2009–2013.                                                    Tok201
08327+2026 ZHN   3     Primary is eta Cas. First known wide pair comprised of an L dwarf and           
                       a giant.                                                                Zhn2010 
08327-5528 HDS1221     Aa = V470 Car, eclipsing binary of Algol type, period 2.16178 days.     Zas2015
08329-0933 J  2642     RST 4407 = LDS 851.                                                             
08331-2436 BU  205     AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 2.73 +/- 0.84, 2.64, and 1.74 Msun, respectively.  Mlk2012 
08332+3326 STF1240     AB: SEI 504.                                                            Nsn2017b
08333-1204 GWP1039     ABL 215.                                                                Tob2012b
08336-0601 GWP1040     ABL 216.                                                                Tob2012b
08338+1104 BPM 446     [PM2000]  894559 + [PM2000]  894443.                                    Gvr2010 
08339-2842 COO 282     SWR  50.                                                                        
08343-1216 GWP1043     ABL 217.                                                                Tob2012b
08344+1557 BPM 447     [PM2000]  895177 + [PM2000]  895164.                                    Gvr2010 
08344-4430 DON 263     CPD-44@2755.                                                                    
08345-3236 FIN 335     Giant primary according to isochrone fit.                                       
                       Hipparcos parallax 14.86 +/- 0.57 mas. Dynamical parallax 14.6 mas,             
                       masses 1.71 and 1.54 Msun.  We confirm and slightly correct the orbit           
                       by Soderhjelm (1999). The 17.35y period is very well defined now, but   Sod1999 
                       further coverage by speckle is still needed. The system is evolved,             
                       judging from its luminosity, estimated masses, and spectral type G5IV.          
                       The speckle dy is very consistent and preferred to dHp.                 Tok2012b
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.24 +/- 0.65, 2.42, and 1.07 Msun, respectively.             Mlk2012 
                       Docobo & Andrade (2013) derive a dynamical parallax of 15.42 +/- 0.28           
                       mas and component masses 1.47 +/- 0.10 and 1.35 +/- 0.09 Msun (for              
                       spectral type G5V) or 16.24 +/- 0.39 mas, 1.26 +/- 0.11 and 1.15 +/-            
                       0.10 Msun (for G5IV). See paper for extensive notes on this system.     Doc2013d
08345-3737 I   195     Variable.                                                                       
08348+1107 BPM 448     [PM2000]  895729 + [PM2000]  895613.                                    Gvr2010 
08354+6746 LDS2283     LDS5198.                                                                        
08354+6616 STF1232     B is BD+66@559.                                                                 
08356+3116 SEI 505     Neither component seen on POSS plate; may be flaws on AC Potsdam plate          
08356+1024 BPM 449     [PM2000]  896580 + [PM2000]  896563.                                    Gvr2010 
08356-0648 LDS3800     Aka GWP1046 and ABL 218.                                                Tob2012b
08358+0637 STF1245     GJ 9271. Visual pair has estimated period of 2500y.                     Tok2006 
                       AB: HJL  95.                                                            HJL1986 
                       HIP 42172. B = HIP 42173.                                               Tok2011a
                       AB: H 3  49.                                                            MEv2010 
                       AB: A is SB2, P=14.296d                                                 Tok2014d
08360+2050 BOV  29     Praesepe VL 184 = NGC 2632 BDA 1184                                             
                       SB1, P = 1:23 d                                                         Bov2001 
08360-1027 GWP1048     ABL 219.                                                                Tob2012b
08360-2211 B  2182     CPD-21@3748.                                                                    
08360-5337 LPO  70     Spectrum: G2/5(III)+A.                                                          
08361-0334 LDS6217     A may be a close double, 50 deg., 2", mag. diff. 0.7.                   Luy1979 
                       NLTT 19864/19867                                                        Chm2004 
08362+1347 STTA 94     B is BD+14@1930.                                                                
08362+1344 BPM 450     [PM2000]  897256 + [PM2000]  897210.                                    Gvr2010 
08363+1933 BOV  30     Praesepe KW 533 = NGC 2632 BDA 533                                              
                       SB2, long period                                                        Bov2001 
08364+3703 SEI 506     Duplicity not apparent on POSS plate; one component may be either               
                       variable star or flaw on AC Potsdam plate.                                      
08364-0306 RST4413     J 1528.                                                                         
08366-1540 GWP1049     ABL 220.                                                                Tob2012b
08367+1643 BPM 451     [PM2000]  897859 + [PM2000]  897884.                                    Gvr2010 
08368+7443 STT 192     A is a spectroscopic binary.                                                    
                       Additional notes may be found in Baize (1939).                          Baz1939a
08369-1154 GWP1050     ABL 221.                                                                Tob2012b
08369-3050 I    68     Spectrum: A3mA7-F2/3.                                                           
08369-7857 KOH  79     KOH  80.  EG Cha.  Wide pair is likely a chance alignment.              Bnk2006 
                       AB: Koehler & Petr-Gotzens (2002) calculate two possible orbital        Koh2002 
                       solutions. The short-period solution gives a semi-major axis of 15.5au          
                       and a mass sum of 2.1 Msun; the longer-period solution gives 37.6au             
                       and 2.3 Msun.                                                                   
08372+2017 BOV  31     Praesepe KW 540 = NGC 2632 BDA 540                                              
                       SB1, P = 1149 d                                                         Bov2001 
08372-4147 CPO 218     TDS5986.                                                                        
08374-0400 GWP1051     ABL 222.                                                                Tob2012b
08375-5336 HJ 4123     B is CPD-53@1782.                                                               
08377+1931 HJ  454     A is a Delta Scuti-type variable.                                               
08377+0542 BUP 118     del Hya = 4 Hya. A spectroscopic binary.                                        
08378+1409 HLD  97     Position corrected by Heintz                                            Hei1983a
08379-0648 HJ   99     AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
08379-2615 RST2571     eta Pyx                                                                         
           VIG  11     The C, E, and F components all appear to be faint background stars;             
                       the D component appears to be co-moving. The mass of D is estimated at          
                       0.07-0.11 Msun.                                                         Vig2012 
08380-0736 GWP1054     ABL 224.                                                                Tob2012b
08380-1750 GWP1053     ABL 223.                                                                Tob2012b
08380-2739 TOK 124     HIP 42344. The ANDICAM position in the V-band is not accurate. NOMAD:           
                       PM(B)=(0,+28), V=16.70, but B is definitely physical. PM(A)=(-147,+95)  Tok2011a
08381+1959 BOV  34     Praesepe KW 79 = NGC 2632 BDA 79                                                
                       Photometric binary                                                      Bov2001 
08382+1922 BOV  35     Praesepe KW 90 = NGC 2632 BDA 90                                                
                       Photometric binary                                                      Bov2001 
08382+1511 RDN   3     Radigan et al. (2013) determine that A and BC appear to share common            
                       proper motion and conclude all components are physically associated.            
                       Derived distance (spectroscopic parallax) is 49 +/- 12 pc. Derived NIR          
                       spectral types and masses (for ages 3 Gyr and 300 Myr) are:                     
                       A  T3   +/- 1   0.060 +/- 0.009 Msun   0.020+/- 0.005 Msun                      
                       B  T3   +/- 1   0.055 +/- 0.008        0.018+/- 0.005                           
                       C  T4.5 +/- 1   0.050 +/- 0.008        0.016+/- 0.004                   Rdn2013 
08386-0249 GWP1056     ABL 225.                                                                Tob2012b
08386-3505 JSP 286     Also known as RSS 167.                                                          
08388-1315 SHY 201     HIP  42401 + HIP  41662.                                                        
08388-3352 B  1621     1995.1160: Quadrant determined by speckle imaging analysis.             Hor1996 
08389-1002 GWP1057     ABL 226.                                                                Tob2012b
08391+2000 HD  73430   Praesepe KW 143 = NGC 2632 BDA 143                                              
                       Praesepe cluster member and occultation binary. Peterson & White        Pts1984 
                       (1984) found a vector separation in April 1982 of 0".044, which should          
                       have been resolvable by us unless the system closed. They find                  
                       magnitude differences (noted as unreliable) of 2.5 mag at 445 nm and            
                       0.35 mag at 750 nm, which if correct would not have prevented us from           
                       seeing the companion.  Incorrectly noted as HD 73460 in text, although          
                       the tabular information is correct.                                     Msn1993b
08391+1418 BPM 452     [PM2000]  900491 + [PM2000]  900455.                                    Gvr2010 
08391-2240 BU  208     CPD-22@3750. Newburg finds little evidence for the perturbation         Nbg1968b
                       suspected by Hirst (1943).                                              Hir1943d
                       AB: A is suspected SB, P=106d? (Abt & Willmarth 2006). Fuhrmann (2011   AbH2006 
                       MNRAS 411, 2311)says Aa,Ab has period few hundred days.                 Tok2014d
                       AC: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
08391-5557 HU 1443     A,BC is a triple system. We provide the first very tentative orbit for          
                       the outer binary, but note its large residuals from the recent                  
                       measures of AB. Strictly speaking, the orbit should describe the                
                       motion of the center-of-gravity of BC around A, rather than the                 
                       measures of AB. Such refinement was made for the orbit of A 2592 AB             
                       (17156-0949)}, but it is not warranted for this preliminary orbit.      Tok2015c
08391-7023 DON 271     the Vol                                                                         
           HJ 4134     AC: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
08392-0317 GWP1060     ABL 227.                                                                Tob2012b
08392-4025 B  1623     Eggen (1982) assigns this star to a group associated with the cluster   Egg1982 
                       IC 2395 at distance of 0.8 kpc.  The Hipparcos Catalogue contains a     HIP1997a
                       light curve with a period of 1.46 d.                                    Msn1998a
                       Includes NX Vel, an Algol type eclipsing binary, P = 2.91992d.          Zas2012 
                       NX Vel is a quadruple system formed by the 0.65" pair, that contains            
                       an eclipsing pair (Otero 2003, IBVS 5480, 1; P~2.9d) and an SB (Sota            
                       et al. 2014, ApJS 211, 10; P=20.6d).                                    Sna2014 
08394-0935 RST4415     Algol (EA) type eclipsing binary, P = 92.1711 d.                        Zas2011 
08394-3636 I   314     Only elements P, T, and a of Heintz (1968) were adjusted for            Hei1968a
                       Starikova (1981) solution.                                              Sta1981a
                       Hipparcos astrometric solution adopted some elements from the orbit of  HIP1997d
                       Heintz (1968).                                                          Hei1968a
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.79 +/- 0.50, 2.01, and 1.51 Msun, respectively.             Mlk2012 
08395-2100 RST5506     CPD-20@3936.                                                                    
08397+2005 COU  47     In Praesepe.                                                                    
08397+0546 STF1255     AB: HJL  96.                                                            HJL1986 
                       AB: H 4  54.                                                            MEv2010 
08397-2934 HJ 4120     zet Pyx. B is CD-29@6545.                                                       
08399+1933 BU  584     In Praesepe.                                                                    
                       DC: D is variable. Position (2000): 08 39.8 +19 32. In Praesepe.                
           S   571     STTA 95. C is a spectroscopic binary, and is +20@2153.                          
                       AC: HJL  97.                                                            HJL1986 
           CHR 156     Da: No published evidence of RV variation. Noted as occultation binary          
                       by Peterson & White (1984). Magnitude differences of 3.1 in blue and    Pts1984 
                       Magnitude differences of 3.1 in blue and 3.8 in red reported by                 
                       Peterson et al. (1989) are consistent with our difficulty in detecting  Pts1989 
                       the faint secondary. Praesepe cluster member.                           Msn1993b
08400-5303 HJ 4126     A is a spectroscopic binary, and is variable.                                   
08401+2000 ENG  37     A: 39 Cnc. A variable?                                                          
           CHR  28     B: 40 Cnc. Praesepe cluster member with excess luminosity. The                  
                       1986.8922 measure is from reanalysis of archival data. Frequently               
                       unresolved, due to large delta m.                                       Msn1993b
08401-3518 RST4894     bet Pyx. A is a spectroscopic binary.                                           
08401-7218 GLI 100     Spectrum: G8/K0III+A.                                                           
08402+5147 OPI  16     AC: The C component is the primary of 08404+5145 ES  909AB.                     
08404+5145 ES  909     The primary is also the C component of 08402+5147 OPI  16AC.                    
08403+1947 BOV  41     Praesepe KW 275 = NGC 2632 BDA 275                                              
                       Photometric binary                                                      Bov2001 
08403+1921 CHR 130     Praesepe cluster member with anomalous occultation behavior (Appleby            
                       1980 JBAA, 139, 1139). The 1984.0607 and 1986 measure are from                  
                       reanalysis of archival data. Peterson et al. (1989) measured            Pts1989 
                       magnitude differences of 1.9 in blue and red.                           Msn1993b
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 13.18 +/- 7.09, 4.10, and 1.51 Msun, respectively.            Mlk2012 
08403-4358 CPO 222     CPD-43@2853.                                                                    
08404+5145 ES  909     The primary is also the C component of 08402+5147 OPI  16AC.                    
08404+1940 STF1254     Algol (EA) type eclipsing binary,  per 7.2209 d.                        Zas2011 
                       Physical with BD+20@2158. A is a spectroscopic binary.                          
           BOV  42     Ba. Praesepe KW 287 = NGC 2632 BDA 287                                          
                       SB1, P = 7635 d                                                         Bov2001 
08404-0641 GWP1063     ABL 228.                                                                Tob2012b
08404-4223 DUN  72     B is CD-41@4370.                                                                
08405+2019 BOV  45     Praesepe KW 297 = NGC 2632 BDA 297                                              
                       SB1, long period                                                        Bov2001 
08405+1933 S   574     eps Cnc = 41 Cnc, a spectroscopic binary. B is BD+20@2163.                      
08405-2255 BRT1466     CD-22@6471.                                                                     
08406-5946 JSP 295     A is a spectroscopic binary and variable, V343 Car.                             
08407+1940 Praesepe... Praesepe KW 322 = NGC 2632 BDA 322                                              
                       SB1, P > 10 000 d                                                       Bov2001 
08408+1940 BOV  47     Praesepe KW 334 = NGC 2632 BDA 334                                              
                       Photometric binary                                                      Bov2001 
08408-1605 GWP1065     ABL 229.                                                                Tob2012b
08408-4504 SNA   6     The primary is the high-mass X-ray binary LM Vel. This O8.5Ib-II(f)             
                       star presents RV variations (Barba et al. 2006, The Astronomer's                
                       Telegram 819, 1) and is an SB candidate. It has been suggested as the           
                       possible counterpart of the fast X-ray transient IGR J08408-4503                
                       (Masetti et al. 2006, The Astronomer's Telegram 819, 1).                Sna2014 
08411+1904 BOV  48     Praesepe KW 365 = NGC 2632 BDA 365                                              
                       Triple, A: SB1O, B: single                                              Bov2001 
08411-0430 GWP1066     ABL 230.                                                                Tob2012b
08412-3005 B  1105     Spectrum: B8/9II/III.                                                           
08413+7614 MLR 548     Also known as TDS6037.                                                          
08413+2029 BU  585     Spectroscopic binary. Praesepe cluster member.                                  
                       1991.3184: Although the peak remains convincing, we  have been unable           
                       to confirm this measure, perhaps due to either a variable secondary or          
                       to the star closing within our resolution limit.                        Msn1993b
08413-1646 GWP1067     ABL 231.                                                                Tob2012b
08413-7858 BNK   3     AB: eta Cha. Likely a chance alignment object.                          Bnk2006 
           SHY 528     AC: HIP  42637 + HIP  42794.                                                    
           BNK   7     CD: The primary of 08432-7904 BNK   7 was found to be the C component           
                       of 08413-7858 SHY 528AC. As the AC pair appears physical, the systems           
                       were merged.                                                                    
                       CD: RS Cha. Likely a chance alignment object.                           Bnk2006 
08414+6426 LDS2288     LDS5199.                                                                        
08414-1927 RSS 169     CPD-19@3721                                                                     
08414-4732 RST 341     CPD-47@2539.                                                                    
08414-5736 JNN  62     The two components of this system have nearly equal colors and                  
                       brightnesses, hence they very likely form a physical pair, although             
                       they have not yet been tested for common proper motion.                 Jnn2012 
08416-7904 BNK   4     EH Cha. Likely a chance alignment object.                               Bnk2006 
08417-1237 ALD  39     BRT 2711.                                                                       
08417-1557 HJ 4124     9 Hya.                                                                          
08417-2018 J  2645     CPD-19@3728.                                                                    
08418+1952 HD  73974   Praesepe KW 428 = NGC 2632 BDA 428                                              
                       Praesepe K0 giant and occultation binary.  Peterson & White (1984)      Pts1984 
                       found a projected separation in April 1982 of 0".018, which could lead          
                       to a true separation below our resolution limit.                        Msn1993b
08419+3546 SEI 508     Secondary not seen on POSS plate; may be either variable star or flaw           
                       on AC Potsdam plate.                                                            
08421-1552 GWP1068     ABL 232.                                                                Tob2012b
08421-4256 EGN   8     C and D components are both background stars.                           Egn2007 
08421-4543 DON 272     CPD-45@2858.                                                                    
08421-5245 B  1624     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.98 +/- 0.24, 1.96, and 0.98 Msun, respectively.             Mlk2012 
08421-6200 HRG  18     Spectral type F8?                                                               
08423-4806 RST5304     A variable, HX Vel.                                                             
08424-5307 BSO  18     A is a variable, HY Vel. B is CD-52@1605.                                       
                       A is a variable, HY Vel. B is CD-52@1605.                                       
           B  1625     BC: Position 08 42.3 -53 06.                                                    
08424-7904 BNK   5     EI Cha. Likely a chance alignment object.                               Bnk2006 
08425-0830 H 6 107     H VI 107. B is BD-08@2463.                                                      
08427+0935 ST    8     KUI.                                                                            
           LUY6218     AB,C: SHY  48. Bayesian analysis by Shaya & Olling (2011) indicates     Shy2011 
                       very high (near 100%) probability pair is physical.                             
08431+1926 BOV  53     Praesepe KW 495 = NGC 2632 BDA 495                                              
                       Triple, A: single, B: SB2                                               Bov2001 
08431-7905 BNK   6     EM Cha. Likely a chance alignment object.                               Bnk2006 
08433+2128 ENG  38     43 Cnc = gam Cnc = Asellus Borealis. A is a spectroscopic binary.               
                       B is BD+21@1897.                                                                
08433-3908 GC 12009    Hipparcos astrometric solution assumed circular orbit (e = omega = 0)   HIP1997d
08433-7905 BNK   8     ET Cha. Both companions are likely chance alignment objects.            Bnk2006 
08434-2743 TDS6057     SWR  53. CPM pair                                                       Skf2004 
08437-0031 GWP1070     ABL 233.                                                                Tob2012b
08437-0714 S   579     B is BD-06@2707.                                                                
                       AB: H 6  82.                                                            MEv2010 
08437-2316 BRT1468     CD-22@6539.                                                                     
08438-1923 GWP1071     ABL 234.                                                                Tob2012b
08438-5038 BRT 743     CPD-50@1746.                                                                    
08439+8614 STF1150     Distance uncertain.                                                             
08439+1902 BLL  26     A is an Algol-type system, S Cnc.                                               
08441-0412 A   552     Orbital motion. A difficult pair, < 0.1" in 1953, 1954.                         
08441-1506 GWP1072     ABL 235.                                                                Tob2012b
08442+0414 BAL2823     Measure by Sil1931 was incorrectly identified as 08465+0419STF1267.     Sil1931 
08443-1327 J  2062     BRT 2712.                                                                       
08443-4544 DON 277     CPD-45@2933.                                                                    
08443-7859 BNK   9     EN Cha. Wide companion is likely chance alignment.                      Bnk2006 
08444-5957 HJ 4139     B is CPD-59@1097.                                                               
08445+2827 STF1266     BDS 4792, H IV 118 same star.                                                   
                       H 4 118.                                                                MEv2010 
08445-6550 EHR  12     Physical/optical nature of AB and AC both undefined.                    Ehr2010 
           TOK 520     AD: D component is the primary of 08465-6605 RST 354.                           
08445-7850 BNK  10     EO Cha. Likely a chance alignment object.                               Bnk2006 
08446-3758 JSP 298     The B component is a likely cataclysmic variable and may be optical.            
08446-4541 DON 279     TDS6073 (merged 2008/06/25)                                                     
08447+1809 TOK   3     Aa,Ab: del Cnc = 47 Cnc = Asellus Australis.                                    
           HJ  457     AB: Optical pair, based on study of relative motion of the                      
                       components using the method of apparent motion parameters.              Kiy2008 
08447-2126 HDS1260     AB + TOK 395: Like WDS 08021-1710, the late-type nearby binary HDS              
                       1260 was discovered by Hipparcos and is expected to move rapidly (HIP           
                       42910, BD-20 2665). It was targeted at SOAR for the first time. To our          
                       surprise, the object turned out to be a resolved triple, with the               
                       secondary being a 0".16 pair of equal stars. Hipparcos failed to                
                       recognize the triple nature of this star. The estimated period of BC            
                       is 15yr. The outer pair AB has closed from 0".8 to 0".5 and moved in            
                       position angle since its discovery. The separations between components          
                       are comparable, so this triple system may be interesting dynamically.   Tok2015c
08447-4117 I   815     CPD-40@2823.                                                                    
08447-4238 CHR 238     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.36 +/- 0.77, 1.84, and 0.85 Msun, respectively.             Mlk2012 
08447-5443 I    10     AB: del Vel.                                                                    
                       The close pair of Tango et al. (1979), originally thought to be a new   Tng1979 
                       close pair (and called TNG 1), was determined to be the Innes pair              
                       with a reflection around the E/W axis.  This problem was first noticed          
                       by Mike Kerr in a private communication to B. Mason.                            
                       Quoted errors in P and a are +14/-11y, +0".03/-0".01.                   Ary2002b
                       AB: Kervella et al. (2013) measured separations between the A and B             
                       components, then based on their orbit of AB derived apparent                    
                       displacements of the center of light of the eclipsing Aa,Ab pair.       Krv2013 
           KEL   1     Aa,Ab: Eclipsing binary. Interferometric solution by Kellerer et al.    Kel2007 
                       (2007), using data from the VLTI/VINCI (K-band, 155m baseline) taken            
                       in April/May 2003. Semimajor axis given as (5.4 +/- 0.5) x 10^10 m,             
                       converted to mas using parallax of 40.90 mas. Aa and Ab are thought to          
                       be of spectral types A0V and A1V, but model fit yields stellar                  
                       diameters of 6.0 +/- 0.5 and 3.3 +/- 0.6 Dsun, larger than would be             
                       expected for main-sequence stars. Authors also conclude that C and D            
                       components of the system are much further away than Aa+Ab+B, so are             
                       not physically associated with the close triple.                                
                       Aa,Ab: Properties of components Aa, Ab, and B are as follows:                   
                       Spectral types: A2IV           A4V            F8V                               
                       M/Msun:         2.5  +/- 0.1   2.0  +/- 0.1   1.3  +/- 0.1                      
                       L/Lsun:         59.2 +/- 2.0   20.0 +/- 0.7   3.1  +/- 0.2                      
                       R/Rsun:         3.17 +/- 0.08  2.02 +/- 0.05  1.39 +/- 0.06                     
                       Teff (K):       9000 +/- 400   8600 +/- 350   6350 +/- 350              Krv2009 
                       Aa,Ab: Masses 2.43 +/- 0.02 and 2.27 +/- 0.03 Msun, luminosities                
                       67. +/- 1. and 51. +/- 1. Lsun, parallax 39.8 +/- 0.4 mas                       
                       Mass sum (Aa+Ab+B) = 6.15 +/- 0.23 Msun, assuming derived parallax.     Mrd2011 
           SHY  49     AF: HIP  42913 + HIP  43797.                                                    
08448+5532 PIN   4     Primary is variable star LT UMa.                                                
08448-0110 GWP1075     ABL 236.                                                                Tob2012b
08449-4050 WG  111     BRT 744.                                                                Brt1933 
08452+4140 STF1263     B is BD+42@1923.                                                                
                       AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
08453-0018 HEI 147     Heintz believes Aitken and van den Bos may have observed this pair              
                       instead of +00@2380.                                                    Hei1983a
08453-0236 STF1270     HJL  98.                                                                HJL1986 
                       HIP 42951. Very small PM(A)=(+1,-9). B is considered physical based on          
                       the CMDs and its brightness.                                            Tok2011a
                       A = MX Hya, Algol, EA type, depth 0.5mag.  Rucinski (2002 PASP 114,             
                       1124) gives period of MX Hya 0.7960d. So far, no estimates of the mass          
                       ratio for Aa,Ab, no SB orbit. dHp=0.49mag.                              Tok2014d
08453-0432 GWP1076     ABL 237.                                                                Tob2012b
08454+6001 MLB 163     LDS1218.                                                                        
08459-0032 GWP1078     ABL 238.                                                                Tob2012b
08460+6945 LDS1681     NLTT 20128/20129                                                        Chm2004 
08460+6445 VBS  42     Incorrectly identified as H 4  60 in BDS. Error noted by MacEvoy.       McE2010 
08461+0748 J   735     B brighter than A in K, redder. A,B both on the MS. B could be SB2.     Tok2014d
08461-0230 ITF  83     Aka ITF  86.                                                                    
08461-4653 CPO 232     CPD-46@2963.                                                                    
08462+1915 STF1269     Chevalier's separation is actually 11".58 rather than 23".68. This      Che1908 
                       pair is identical with STF1269, but the incorrect published value for           
                       led to a match with a nearby pair which roughly agreed with the                 
                       Chevalier measure, and its publication as 08467+1914 CHE 507. Measures          
                       have been merged.                                                       Hrt2012b
08464-0852 GWP1079     ABL 239.                                                                Tob2012b
08464-1333 RST5507     12 Hya. A is a spectroscopic binary.                                            
08464-1413 BRT2713     J 2887.                                                                         
08465+6437 LDS2292     LDS5200.                                                                        
08466-4234 JC   13     Also classed B4V.                                                               
08467+2846 STF1268     iot Cnc. B is BD+29@1823, spectral type A3V.                                    
                       HJL  99.                                                                HJL1986 
                       H 4  52.                                                                MEv2010 
08468+0625 SP    1     eps Hya = 11 Hya. Variable.                                             Dan1952 
                       The elements for AB are combined visual-spectroscopic.                  Hei1963c
                       A secondary radial velocity variation with a period of about 70d                
                       was suspected by Underhill (Pub. DAO Victoria 12, 161, 1963)            Fin1970b
                       See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
           STF1273     C is SB1, P = 9.905 d.                                                          
                       AB,C triple solution ((AB)-C in HIP).                                   Sod1999 
                       Star D is in slow direct motion, hence quintuple.                               
08468-0219 GWP1080     AB: ABL 240AB.                                                          Tob2012b
           GWP1081     AC: ABL 240AC.                                                          Tob2012b
08469+4225 LDS3816     NLTT 20202/20201                                                        Chm2004 
08469+1753 CUD   4     Central star of the planetary Nebula Abell 30.                                  
08470-3846 B  2186     The nf star of CD-38@4867.                                                      
08471-0747 GWP1082     ABL 241.                                                                Tob2012b
08471-4032 WG  114     CPD-40@2867.                                                                    
                       Possible typo in the AC catalog used to generate the WG measure. The            
                       AC2000 coordinates in Aladin agree with the WG measure, but the                 
                       secondary coordinate and the actual star position are about 20" apart,          
                       due north-south of each other.                                                  
08474-4143 CPO 233     CPD-41@2968.                                                                    
08476+0001 STF1281     AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
           RST5306     The C component of 08476+0001. WDS designation changed from 08476+0005          
                       and this pair given component designations Ca,Cb.                               
08476-0721 GWP1085     ABL 242.                                                                Tob2012b
08476-1859 LDS 235     NLTT 20261/20260                                                        Chm2004 
08477-4144 MUG   6     Theta approximate ("east"). Based on relative motion between 1999               
                       2MASS data and two measures with NTT in 2002, Mugrauer et al. (2004)    Mug2004b
                       conclude the B component is a CPM companion to the planet host star             
                       HD 75289. Assuming distance of 28.94 +- 0.47pc, this corresponds to a           
                       separation of 621 au. Mass of B ~0.135 +- 0.003 Msun. Additional                
                       photometry and astrometry compiled from 2MASS catalog.                          
                       Exoplanet host, P=3.5d. Large motion (diff. with 2MASS). Optical?               
                       Roell et al. (2012 A&A 542, A92) consider B physical (no PM), as do     Rag2006 
                       Raghavan et al. (2006).                                                 Tok2014d
08479-7855 BNK  11     EQ Cha. Koehler & Petr-Gotzens (2002) suspected duplicity but were      Koh2002 
                       unable to split the pair.                                                       
                       More commonly known as EQ Cha, this star appears single in the                  
                       AstraLux images, but has most likely been partially resolved as close           
                       binary in previous imaging campaigns (Kohler & Petr-Gotzens 2002;       Koh2002 
                       Brandeker et al. 2006). With an angular separation as small as 40 mas   Bnk2006 
                       in 2003, it is fully plausible that the companion exists but was too            
                       close to be resolved by AstraLux in 2010.                               Jnn2012 
08480-3115 SHY 529     AC: HIP  43193 + HIP  43316.                                                    
08481+1757 BPM 453     [PM2000]  909715 + [PM2000]  909682.                                    Gvr2010 
08481-0647 GWP1086     ABL 243.                                                                Tob2012b
08484+0550 AGC   3     rho Hya = 13 Hya. A is a spectroscopic binary, P = 8.2d.                        
08485+1449 BPM 454     [PM2000]  910131 + [PM2000]  910071.                                    Gvr2010 
08486+0237 A  2551     Rapid motion. Quadrant ambiguity, but it appears that at least one              
                       revolution is complete.                                                         
08486-1353 JNN  64     B: LP 726-12.                                                                   
                       Ba,Bb: 2MASS J08483696-1353087 and J08483645-1353083 are separated by           
                       only 7", the former is a close binary (as of yet unconfirmed by common          
                       proper motion) and the latter is single, so this is likely a triple             
                       system in reality.                                                      Jnn2012 
08487+0057 A  2552     Aitken's angles 1913-1935 should all be put in the third quadrant.      B__1963b
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.29 +/- 0.91, 2.59, and 1.20 Msun, respectively.             Mlk2012 
08494-6216 HJ 4147     CD-61@2042.                                                                     
08495-2054 J  1532     08496-2055ARA1061.  Hyderabad -21@ 8h 44m, Nos 43175-176.                       
08497-0852 GWP1087     ABL 244.                                                                Tob2012b
08497-4249 RSS  10     This previously uncataloged double star was a Hipparcos double entry            
                       system.  The first measure is determined from the individual positions          
                       listed by Rousseau et al.                                               Rss1996 
08499+1450 STF1283     H 4 111.                                                                MEv2010 
08499-1928 GWP1089     ABL 245.                                                                Tob2012b
08500+1155 BPM 455     [PM2000]  911727 + [PM2000]  911657.                                    Gvr2010 
08500-0322 GWP1090     ABL 246.                                                                Tob2012b
08502+1219 HJ 2469     Not found by Heintz at IDS position.                                    Hei1990b
08502-0214 J  2065     BAL 512.                                                                        
08503+1057 SKF 363     Aa,Ab: NLTT 20346. Faherty et al. (2011) derive distance estimates for  Fah2011 
                       Aa and Ab of 28 +/- 5 and 33 +/- 5 pc, respectively, and estimate               
                       spectral types at M5 +/- 0.5 and M6 +/- 0.5.                                    
           FAH   1     AB: Faherty et al. (2011) also determine a distance for RED 10 of 29    Fah2011 
                       +/- 7 pc; similar distance and proper motions indicate SKF 363 and              
                       RED 10 form a likely CPM pair at a distance of 248".                            
           RED  10     Ba,Bb: 2MASSs J0850359+105716                                                   
                       Ba component is an L6V brown dwarf; LRIS spectrum shows that other              
                       component is a background M star.                                       Kir1999 
                       Reid et al (2002) observations from HST and WFPC2. Paper includes mass  Red2001 
                       and age estimates, as well as discussion of L dwarf binary frequency            
                       and semimajor axis distribution.                                                
                       Burgasser et al. (2011) derive spectral types of L7 and L6, masses      Bug2011 
                       0.06 +/- 0.02 and 0.05 +/- 0.02 Msun, effective temperatures                    
                       1770 +/- 200 and 1400 +/- 170K.                                                 
                       Ba,Bb: Assuming a parallactic distance of 38.1 +/- 7.3 pc                       
                       (Vrba et al. 2004), Konopacky et al. (2010) derive a system mass of     Vrb2004 
                       0.2 +/- 0.2 Msun.                                                       Kon2010 
08503+0125 J    74     Pair measured in 1947 is indeed the BD+01 2181 observed previously.             
                       Pair is -42s, +4' from BD+02 2072. movement is perhaps rectilinear.     J__1949a
08503-0156 J  1350     BAL 513. J 2595.                                                                
08503-4349 CPO 236     CPD-43@3034.                                                                    
08504+1123 HJ 2470     CHE 114. Chevalier pair originally copied to catalog with 10' error in          
                       declination (08504+1133).                                                       
08504-0002 HJ 3314     HJL 100.                                                                HJL1986 
08504-0210 J  1533     BAL 514.                                                                        
08504-0440 GWP1091     ABL 247.                                                                Tob2012b
08504-4205 SNA   7     The object is marginally resolved with rho~0.5mas, although with large          
                       relative uncertainty. Given the distance of 947pc (Sota et al. 2014,            
                       ApJS 211, 10) this pair probably  corresponds to the known SB2                  
                       (P=33.1d, a1+a2 sin i = 0.6au; Thackeray et al. 1966, MNRAS 134, 97).   Sna2014 
                       The classification is from Thackeray (1966 MNRAS 134, 97).  The star    Egg1982 
                       is part of a group associated with the cluster IC 2395 (Eggen 1982)     Msn1998a
08505+2308 AG  157     At some time between 1961 (IDS) and the 1984 version of the WDS, the            
                       two Espin pairs 23505+5023ES  926AC and AD were erroneously also added          
                       to this system as 08505+2308ES 2630AC and AD. The reason is unknown.    Es_1910b
08505-3813 JSP 307     A is variable.                                                                  
08506+1211 CHE 115     Based on a check of coordinates for other objects flagged as                    
                       Durchmusterung stars, Chevalier’s coordinates are very accurate for     Che191
                       this plate. There are no obvious errors in applying the offset from             
                       the plate center, but there are no pairs at Chevalier’s coordinates,    .     
                       nor at coordinates found by reversing the sign of either or both                
                       offsets.  The pair is likely lost.                                      Hrt2012b
                       Coordinates found to be off in dec by ~9arcmin.                                 
08506-4632 HDO 205     The classification is from Conti et al. (1977).  Part of an eclipse     Cti1977 
                       was observed by Balona & Laing (1986 MNRAS 223, 621); the orbital               
                       ephemeris is discussed by Mayer et al. (1997 A&A 320, 109).             Msn1998a
                       The primary is the variable star KX Vel.                                        
08507+1800 A  2473     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 72.60 +/- 61.48, 7.81, and 0.95 Msun, respectively.           Mlk2012 
08507+0752 VDK   3     A premature orbit has been computed.                                    Cou1953d
08508+1143 BPM 456     [PM2000]  912512 + [PM2000]  912473.                                    Gvr2010 
08509+1152 BPM 457     [PM2000]  912707 + [PM2000]  912762.                                    Gvr2010 
08510+3053 HJ  459     SEI 511.                                                                Nsn2017b
08510+1159 BPM 458     [PM2000]  912736 + [PM2000]  912621.                                    Gvr2010 
08510+1150 BPM 459     [PM2000]  912825 + [PM2000]  912775.                                    Gvr2010 
08510+1148 BPM 460     [PM2000]  912844 + [PM2000]  912913.                                    Gvr2010 
08510-0147 GWP1092     ABL 248.                                                                Tob2012b
08511+1146 BPM 462     [PM2000]  912881 + [PM2000]  912908.                                    Gvr2010 
08511+1145 BPM 463     [PM2000]  912886 + [PM2000]  912785.                                    Gvr2010 
08511-0056 GWP1093     ABL 249.                                                                Tob2012b
08512+1149 BPM 461     BD: [PM2000] 913012  + [PM2000]  912857.                                Gvr2010 
                       Secondary of 08510+1149 BPM 461 found to be secondary of 08512+1149             
                       CHE 118 AB. Systems merged, with quadrant flipped 180deg for BPM 461.           
08512-1448 GWP1094     ABL 250.                                                                Tob2012b
08513+1153 BPM 481     [PM2000]  913301 + [PM2000]  913350.                                    Gvr2010 
08513+1152 BPM 474     [PM2000]  913236 + [PM2000]  913266.                                    Gvr2010 
                       Primary is D component of 08513+1150 BPM 464BD.                                 
08513+1151 BPM 467     BC: [PM2000]  913188 + [PM2000]  913213.                                Gvr2010 
           BPM 468     BD: [PM2000]  913188 + [PM2000]  913337.                                Gvr2010 
08513+1150 BPM 475     AB: [PM2000]  913241 + [PM2000]  913165.                                Gvr2010 
           BPM 476     AC: [PM2000]  913241 + [PM2000]  913284.                                Gvr2010 
           BPM 464     BD: [PM2000]  913165 + [PM2000]  913236.                                Gvr2010 
                       D component is primary of 08513+1152 BPM 474.                                   
08513+1149 BKO  38     AB: B component is H component of 08514+1148 BPM 487BH.                         
           BPM 472     AC: [PM2000]  913227 + [PM2000]  913148.                                Gvr2010 
           BPM 473     AD: [PM2000]  913227 + [PM2000]  913158.                                Gvr2010 
           BPM 483     AE: [PM2000]  913227 + [PM2000]  913343.                                Gvr2010 
           BPM 484     AF: [PM2000]  913227 + [PM2000]  913366.                                Gvr2010 
           BPM 485     EF: [PM2000]  913343 + [PM2000]  913366.                                Gvr2010 
08513+1146 BPM 470     CE: [PM2000]  913215 + [PM2000]  913334.                                Gvr2010 
                       A component is G component of 08514+1146 BPM 466FG.                             
                       E component is C component of 08514+1148 BPM 490AC.                             
08513+1145 BPM 482     [PM2000]  913302 + [PM2000]  913225.                                    Gvr2010 
08513+1144 BPM 465     [PM2000]  913178 + [PM2000]  913328.                                    Gvr2010 
08513+1126 BPM 471     [PM2000]  913217 + [PM2000]  913042.                                    Gvr2010 
08514+1149 BPM 495     [PM2000]  913426 + [PM2000]  913355.                                    Gvr2010 
08514+1148 BPM 489     AB: [PM2000]  913415 + [PM2000]  913379.                                Gvr2010 
           BPM 490     AC: [PM2000]  913415 + [PM2000]  913334.                                Gvr2010 
                       C component is E component of 08513+1146 BPM 470CE.                             
           BPM 491     AD: [PM2000]  913415 + [PM2000]  913345.                                Gvr2010 
           BPM 492     AE: [PM2000]  913415 + [PM2000]  913346.                                Gvr2010 
                       E component is E component of 08515+1151 BPM 505AE.                             
           BPM 493     AF: [PM2000]  913415 + [PM2000]  913566.                                Gvr2010 
           BPM 494     AG: [PM2000]  913415 + [PM2000]  913565.                                Gvr2010 
                       G component is E component of 08515+1149 BPM 515BE.                             
           BPM 487     BH: [PM2000]  913379 + [PM2000]  913251.                                Gvr2010 
                       H component is B component of 08513+1149 BKO  38AB.                             
           BPM 469     HI: [PM2000]  913251 + [PM2000]  913194.                                Gvr2010 
08514+1146 BPM 477     AB: [PM2000]  913292 + [PM2000]  913250.                                Gvr2010 
           BPM 478     AC: [PM2000]  913292 + [PM2000]  913402.                                Gvr2010 
           BPM 479     AD: [PM2000]  913292 + [PM2000]  913277.                                Gvr2010 
           BPM 480     BE: [PM2000]  913250 + [PM2000]  913409.                                Gvr2010 
           BPM 488     CF: [PM2000]  913402 + [PM2000]  913326.                                Gvr2010 
           BPM 466     FG: [PM2000]  913326 + [PM2000]  913184.                                Gvr2010 
08515+1154 CHE 120     B component is H component of 08515+1152 BPM 501CH.                             
08515+1152 BPM 498     CE: [PM2000]  913490 + [PM2000]  913519.                                Gvr2010 
           BPM 499     CF: [PM2000]  913490 + [PM2000]  913553.                                Gvr2010 
           BPM 500     CG: [PM2000]  913490 + [PM2000]  913554.                                Gvr2010 
           BPM 501     CH: [PM2000]  913490 + [PM2000]  913458.                                Gvr2010 
                       H component is B component of 08515+1154 CHE 120.                               
           BPM 513     CI: [PM2000]  913490 + [PM2000]  913570.                                Gvr2010 
                       I component is B component of 08516+1152 CHE 123AB.                             
           BPM 517     EI: [PM2000]  913519 + [PM2000]  913593.                                Gvr2010 
           BPM 518     EJ: [PM2000]  913519 + [PM2000]  913609.                                Gvr2010 
                       J component is C component of 08516+1152 BKO  46AC.                             
           BPM 519     EK: [PM2000]  913519 + [PM2000]  913612.                                Gvr2010 
                       K component is J component of 08516+1152 BPM 520CJ.                             
           BPM 512     FG: [PM2000]  913553 + [PM2000]  913554.                                Gvr2010 
           BPM 514     FI: [PM2000]  913553 + [PM2000]  913570.                                Gvr2010 
           BPM 496     GH: [PM2000]  913554 + [PM2000]  913458.                                Gvr2010 
08515+1151 BPM 502     AB: [PM2000]  913499 + [PM2000]  913468.                                Gvr2010 
                       A component is D component of 08516+1152 BPM 506AD.                             
                       B component is E component of 08516+1152 BPM 521AE.                             
           BPM 503     AC: [PM2000]  913499 + [PM2000]  913471.                                Gvr2010 
           BPM 504     AD: [PM2000]  913499 + [PM2000]  913533.                                Gvr2010 
                       D component is F component of 08516+1152 BPM 522AF.                             
           BPM 505     AE: [PM2000]  913499 + [PM2000]  913346.                                Gvr2010 
                       E component is E component of 08514+1148 BPM 492AE.                             
           BPM 509     BD: [PM2000]  913468 + [PM2000]  913533.                                Gvr2010 
           BPM 486     BE: [PM2000]  913468 + [PM2000]  913346.                                Gvr2010 
           BPM 510     CD: [PM2000]  913471 + [PM2000]  913533.                                Gvr2010 
           BPM 508     DE: [PM2000]  913533 + [PM2000]  913346.                                Gvr2010 
           BPM 526     DF: [PM2000]  913533 + [PM2000]  913681.                                Gvr2010 
                       F component is I component of 08516+1152 CHE 124KI.                             
08515+1149 BPM 515     BE: [PM2000]  913582 + [PM2000]  913565.                                Gvr2010 
           BPM 516     BF: [PM2000]  913582 + [PM2000]  913601.                                Gvr2010 
                       E component is G component of 08514+1148 BPM 494AG.                             
08515+1148 BPM 497     [PM2000]  913486 + [PM2000]  913564.                                    Gvr2010 
08515+1146 BPM 511     [PM2000]  913542 + [PM2000]  913676.                                    Gvr2010 
08515+1135 BPM 507     [PM2000]  913518 + [PM2000]  913560.                                    Gvr2010 
08516+1154 BPM 523     AB: [PM2000]  913647 + [PM2000]  913504.                                Gvr2010 
           BPM 524     AC: [PM2000]  913647 + [PM2000]  913672.                                Gvr2010 
08516+1152 CHE 123     AB: B component is I component of 08515+1152 BPM 513CI.                         
           BKO  46     AC: C component is J component of 08515+1152 BPM 518EJ.                         
           BPM 506     AD: [PM2000]  913614 + [PM2000]  913499.                                Gvr2010 
                       D component is A component of 08515+1151 BPM 502AB.                             
           BPM 521     AE: [PM2000]  913614 + [PM2000]  913468.                                Gvr2010 
                       E component is B component of 08515+1151 BPM 502AB.                             
           BPM 522     AF: [PM2000]  913614 + [PM2000]  913787.                                Gvr2010 
           BPM 531     CH: [PM2000]  913609 + [PM2000]  913690.                                Gvr2010 
           BPM 527     CI: [PM2000]  913609 + [PM2000]  913681.                                Gvr2010 
           BPM 520     CJ: [PM2000]  913609 + [PM2000]  913612.                                Gvr2010 
                       J component is K component of 08515+1152 BPM 519EK.                      .      
           BPM 533     CK: [PM2000]  913609 + [PM2000]  913720.                                Gvr2010 
           BPM 534     CL: [PM2000]  913609 + [PM2000]  913724.                                Gvr2010 
           BPM 537     FG: [PM2000]  913787 + [PM2000]  913894.                                Gvr2010 
           BPM 528     HI: [PM2000]  913690 + [PM2000]  913681.                                Gvr2010 
           BPM 536     HL: [PM2000]  913690 + [PM2000]  913724.                                Gvr2010 
           BPM 535     IL: [PM2000]  913681 + [PM2000]  913724.                                Gvr2010 
           BPM 529     IM: [PM2000]  913681 + [PM2000]  913753.                                Gvr2010 
                       M component is C component of 08516+1147 BPM 532BC.                             
           CHE 124     KI: I component is F component of 08515+1151 BPM 526DF.                         
08516+1147 BPM 525     AB: [PM2000]  913651 + [PM2000]  913713.                                Gvr2010 
           BPM 532     BC: [PM2000]  913713 + [PM2000]  913753.                                Gvr2010 
                       C component is M component of 08516+1152 BPM 529IM.                             
08516+1137 BPM 530     [PM2000]  913687 + [PM2000]  913615.                                    Gvr2010 
08516-0711 BU  587     15 Hya. A is a spectroscopic binary, and one component is variable.             
           H 5 120     AC: H V 120.                                                                    
08517+1144 BPM 538     [PM2000]  913812 + [PM2000]  913815.                                    Gvr2010 
08518+1150 BPM 539     CD: [PM2000]  913923 + [PM2000]  914017.                                Gvr2010 
           BPM 545     DE: [PM2000]  914017 + [PM2000]  913879.                                Gvr2010 
08518+1146 BPM 540     [PM2000]  913948 + [PM2000]  913834.                                    Gvr2010 
08519+6308 KR   32     Also known as LDS2294.                                                          
08519+1205 BPM 542     [PM2000]  913976 + [PM2000]  914014.                                    Gvr2010 
08519+1158 BPM 541     [PM2000]  913972 + [PM2000]  913843.                                    Gvr2010 
08519+1148 BPM 546     [PM2000]  914090 + [PM2000]  914091.                                    Gvr2010 
08519+1141 BPM 544     [PM2000]  914010 + [PM2000]  914054.                                    Gvr2010 
08519+1130 BPM 543     [PM2000]  914004 + [PM2000]  913999.                                    Gvr2010 
08520+2543 STTA 96     B is BD+26@1854.                                                                
08520+1156 BPM 547     [PM2000]  914173 + [PM2000]  914218.                                    Gvr2010 
08521-4751 BRT 754     CPD-47@2847.                                                                    
08522+1144 BPM 548     [PM2000]  914371 + [PM2000]  914387.                                    Gvr2010 
08523+1143 BPM 549     [PM2000]  914522 + [PM2000]  914476.                                    Gvr2010 
08523+0804 TOK  22     Estimated period of visual pair 600y.                                   Tok2006 
                       A is SB1, P=10.25d, Griffin & Fuhrmann 2013 MNRAS, 430, 1390). B is             
                       SB2 (P~10d). Fuhrmann (2005 MNRAS, 361, 803) gave Mass(Aa)=0.96Msun,            
                       age 8.2Gyr, Ab is WD?  However, Griffin & Fuhrman said  P(Aa,Ab)=10d            
                       and tertiary. Ab not a WD. Tok2006: dK=(AB)=4.28 => Mass(Ba)=0.23               
08523-1837 GWP1095     ABL 251.                                                                Tob2012b
08523-1913 GWP1096     ABL 252.                                                                Tob2012b
08525+2816 HJ  460     53 Cnc. A is the variable BO Cnc.                                               
                       C component is A component of 08526+2820 LDS6219.                               
08525+1206 BPM 550     [PM2000]  914773 + [PM2000]  914798.                                    Gvr2010 
08526+3228 HU 1125     sig 1 Cnc = 51 Cnc. A spectroscopic binary.                                     
           S   583     AC: H 6  86.                                                            MEv2010 
08526+2820 LDS6219     55 Cnc = Copernicus.  NLTT 20414/20418                                  Chm2004 
                       A component is C component of 08526+2816 HJ  460AC.                             
           55 Cnc      A: Combined solution, based on reduction of Hipparcos intermediate              
                       astrometric data together with spectroscopic elements from Butler       CPS1997a
                       et al. (1997).                                                          HaI2001 
08526+2527 BRT3289     Originally published as BRT 153.                                        Brt1928 
08526-3633 FIN 296     More than one revolution?                                                       
08527+2231 LDS6220     NLTT 20426/20425                                                        Chm2004 
08530+1625 BPM 551     [PM2000]  915167 + [PM2000]  915161.                                    Gvr2010 
08530-0834 GWP1099     ABL 253.                                                                Tob2012b
08531+5457 A  1584     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.07 +/- 0.60, 2.18, and 1.05 Msun, respectively.             Mlk2012 
08531+1320 BPM 552     [PM2000]  915268 + [PM2000]  915272.                                    Gvr2010 
08531-0437 LDS3828     NLTT 20452/20453                                                        Chm2004 
08531-5639 MWT   2     Mawet et al. (2015) find a companion to HR 3549at ~80au, and determine          
                       that the pair shares common proper motion. The companion has a mass             
                       roughly estimated at 15-80 Mjup.                                        Mwt2015 
08532-0732 GWP1100     ABL 254.                                                                Tob2012b
08533-0356 GWP1101     ABL 255.                                                                Tob2012b
08535-2249 DON 292     J  2066.                                                                J__1962a
08535-4603 CPO 241     CPD-45@3221.                                                                    
08536+1210 GII  38     Ba,Bb: Probably the same as GII  79Ba,Bb. Gili (2016) lists two                 
                       separate pairs of similar separation and position angle, and                    
                       associates both with HEI 480. However, he gives a position and UCAC4            
                       designation for the 2011 measure which correspond to a 16th magnitude           
                       star about 34" east of the Heintz pair.                                 Gii2016 
08536-1722 TOK 666     Resolved with ANDICAM2. A has small PM. AB is considered physical on            
                       photometry only.                                                        Tok2014d
08538-0035 STF1292     BDS 4842, HDO 120.                                                              
                       HJL 101.                                                                HJL1986 
08538-4731 FIN 316     Low incl fixed at 15 deg, Omega=0 for Soderhjelm (1999) orbit.          Sod1999 
                       High mass-sum and q=1.5(0.3) corroborates secondary 9.1d SB2            Wor1983 
                       The primary is SB2, P = 9.07 d. 1912-13 (Lick Obs. Bul. 16, 137,                
                       1928); no later observations.                                                   
                       Hipparcos astrometric solution adopted some elements from the orbit of  HIP1997d
                       Finsen (1973).                                                          Fin1973a
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 4.25 +/- 0.50, 3.21, and 1.58 Msun, respectively.             Mlk2012 
08539+0149 A  2554     Very difficult object, even in good definition, due to magnitude                
                       difference. All 1936-1941 measures noted as very hard and uncertain.            
                       Aitken has two measures in 1913, a very uncertain one in 1923, and              
                       failed to see the companion in 1935.                                    B__1951a
08539-1308 ST    9     L 820-19 = LPM 299 = LDS3829.                                                   
                       NLTT 20496/20497                                                        Chm2004 
08539-2026 RSS 178     CPD-19@3889                                                                     
08539-6648 EGN   9     Single epoch, so bound/unbound nature of pair unknown. Primary is               
                       planet host star.                                                       Egn2007 
08540-0103 GWP1102     ABL 256.                                                                Tob2012b
08540-4229 FGS  24     The classification is from Garrison et al. (1977 ApJS 35, 111).         Msn1998a
08542+3035 STF1291     Mt. Wilson spectral types G7,K0.                                                
                       AB: H 1  30.                                                            MEv2010 
08542-1629 GWP1104     ABL 257.                                                                Tob2012b
08543-3653 BRT1641     SWR  55.                                                                        
08544-0821 GWP1105     ABL 258.                                                                Tob2012b
08546+1219 CHE 134     A star of appropriate magnitude is seen at Chevalier’s coordinates,     Che191
                       but with no companion. Reversing the sign of either or both offsets             
                       from the plate center yields no likely pairs, either. Perhaps the               
                       secondary measured by Chevalier was instead a plate flaw or other               
                       spot on the emulsion?                                                   Hrt2012b
08546-1925 GWP1107     ABL 259.                                                                Tob2012b
08548+4335 STF1289     H 1  85.                                                                MEv2010 
08548-1406 GWP1108     AB: ABL 260AB.                                                          Tob2012b
           GWP1109     AC: ABL 260AC.                                                          Tob2012b
08549+2612 A  2131     See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 2.43 +/- 0.47, 2.30, and 1.85 Msun, respectively.  Mlk2012 
           HO  357     AB,C: Optical pair, based on study of relative motion of the                    
                       components using the method of apparent motion parameters.              Kiy2008 
08550-1205 GWP1110     ABL 261.                                                                Tob2012b
08551-4736 SNA   8     Star is a member of the Vela OB1 association; at the distance of that           
                       association the projected separation of the new pair is 2.3au. The              
                       resolved companion may be the reported spectroscopic companion, if              
                       the spectroscopic period is greater than ~6 months.                     Sna2014 
                       LS 1204. Classification is from Garrison et al. (1977 ApJS 35, 111).    Msn1998a
08552+1612 BPM 553     [PM2000]  917386 + [PM2000]  917319.                                    Gvr2010 
08552-1814 S   585     B is BD-17@2692.                                                                
08553-1122 S   584     B is BD-10@2691.                                                                
08554+7048 STF1280     AB: LDS1684. Mt. Wilson spectral types M0, M0. Proper motion of                 
                       A -1334 -362, B -1364 -407. C -008-020                                          
                       H N 144.                                                                Bu_1906 
08554-4653 RST 361     Includes OV Vel, a Beta Lyr type eclipsing binary, P = 2.09051d.        Zas2012 
08555-0758 STF1295     17 Hya. Both components are metallic-line stars.                                
                       H 2  77.                                                                MEv2010 
08555-2741 SEE 107     del Pyx                                                                         
08557-1531 GWP1113     ABL 262.                                                                Tob2012b
08558+6458 ARG  21     A is an Algol-type system, AC UMa.                                              
08559+4632 LDS 908     NLTT 20526/20527                                                        Chm2004 
08560-0724 GWP1115     ABL 263.                                                                Tob2012b
08562-5532 DUN  73     B is CPD-55@1852.                                                               
08563+1239 JNN 274     G 41-8. Estimated age 30-300 Myr; masses 0.13 +/- 0.08 and 0.11 +/-             
                       0.06 Msun; a ~27.0 au.                                                  Jnn2014 
08563-1908 BRT1471     J 2646.                                                                         
08563-5243 R    87     A is a spectroscopic binary.                                                    
08564-0916 GWP1116     ABL 264.                                                                Tob2012b
08565+7058 HZG   7     Also known as LDS1685.                                                          
08567+1951 BLL  27     A is a semiregular variable, T Cnc.                                             
08568+2235 BOY   2     Aa,Ab: 2MASSI J0856479+223518                                                   
                       Physical companionship to this ultracool dwarf ruled out based on i-z           
                       and z-J colors, using photometry from SDSS.                             AlP2007 
08568-1401 GWP1119     ABL 265.                                                                Tob2012b
08568-1726 SHY 533     BC: HIP  43920 + HIP  44657.                                                    
08568-3205 HJ 4154     SWR  58. CPM pair                                                       Skf2004 
08570-0754 GWP1120     ABL 266.                                                                Tob2012b
08570-5914 DUN  74     A variable, V376 Car.                                                           
08571-2951 TOK  63     Aa,Ab: Estimated masses 0.64 and 0.59 Msun; sep 15.9 au, period 60 y.   Tok2010c
                       Ba,Bb: Estimated masses 0.55 and 0.24 Msun; sep 10.9 au, period 40 y.   Tok2010c
08572+1519 SHY 204     HIP  43970 + HIP  44001.                                                        
08573-0948 GWP1121     ABL 267.                                                                Tob2012b
08575-5045 HD  76968   Turner (1979 A&A 76, 350) includes this star in a group with the                
                       Cepheid SW Vel which lies beyond Vel OB1 at a distance of 2.6 kpc.      Msn1998a
08579-4744 SNA   9     Aa,Ab: The separation changed from 1.5 to 4.1 mas over 5.6 months,              
                       indicating clear orbital motion. The system exhibits non-thermal X-ray          
                       emission (Benaglia et al. 2001, A&A 535, A53), possibly due to                  
                       wind-wind collision in the binary system.                               Sna2014 
08580+3014 HO  252     61 Cnc. Rapid binary? Measures scattered and uncertain.                 Mlr1950a
                       The separation of this partially resolved pair for 1986.388 was                 
                       calculated under the assumption of zero or otherwise known magnitude            
                       difference.                                                             Tok1985 
08580+2428 OSO  23     G009-036. Not a common proper motion pair                               Oso2004 
08581+1130 GIC  82     G046-012/G046-013.                                                              
08581-3852 RSS  11     This previously uncataloged double star was a Hipparcos double entry            
                       system.  The first measure is determined from the individual positions          
                       listed by Rousseau et al.                                               Rss1996 
08582+1945 LDS3836     LSPM J0858+1945 = EI Cnc. Law et al (2008) derive a distance of         Law2008 
                       5.23 +/-0.07 pc and a projected separation of 7.27 +0.11/-0.11 au.              
                       Estimated spectral types are M5.5 and M6.                                       
                       LHS 2077. Estimated age 1000-10000 Myr; masses 0.13 +/- 0.03 and 0.11           
                       +/- 0.02 Msun; a ~9.6 au.                                               Jnn2014 
08584-1422 LDS3837     NLTT 20663/20660                                                        Chm2004 
08585+3548 COU1897     Semi-major axis value of 0".4 in Couteau (1999) appears to have been    Cou1999b
                       a typo. Changed to 0".14 in orbit catalog.                                      
08585+1151 HJ  110     alp Cnc = 65 Cnc = Acubens. A is an occultation double.                         
08586+2711 ZHN   4     NLTT 20640 + 2MASS J08583693+2710518. Baron et al. (2015) estimate              
                       spectral types M4.0 +/- 0.5 and L0 +/- 1, distances 54 +32/-20 and              
                       48 +3/-14 pc, masses 0.207-0.272 and 0.074-0.081 Msun.                  BFr2015 
08589+0829 DEL   2     G 41-14.  A triple system with a close spectroscopic pair on a 7.6 day          
                       orbit, and one wider component which is reported at a separation of             
                       620 mas in Delfosse et al. (1999). Subsequently, an orbit has been      Del1999a
                       determined for the wider pair (Hartkopf et al. 2012), with a period of  Hrt2012a
                       5.66 years and a 424 mas angular semi-major axis. Using the estimated           
                       orbital elements to predict the location of the wider component in Jan          
                       2012 when the AstraLux image was taken, the predicted separation is             
                       ∼100 mas. This is in excellent agreement with what is seen in the       .     
                       AstraLux image, where the PSF is substantially extended, but not quite          
                       sufficiently to get a satisfactory binary fit.                          Jnn2014 
08589-4714 HJ 4161     A is a Delta Scuti-type variable, FZ Vel.                                       
08590+0938 LDS3838     SLW 320.                                                                        
08591+3155 TOK 522     AB is accepted as physical because of large PM(A) and low crowding              
08592+4803 HJ 2477     iot UMa = 9 UMa = Talitha. A is a Delta Scuti-type variable and SB1,            
                       P = 11.03y.                                                                     
                       A,BC: STT 196. A premature orbit has been computed. Quadruple.                  
                       A,BC: While the orbit may be good for ephemerides, system is unstable.  PkO2014 
           HU  628     See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
08593+2006 BRT2396     COU  48.                                                                        
08594-5905 SHY 205     AC: HIP  44143 + HIP  48133. C component = A component of 09488-5237.           
08595+3225 SHJ 100     sig 3 Cnc = 64 Cnc. B is BD+32@1820.                                            
                       AB: H 6  87.                                                            MEv2010 
08595+2918 LAW  16     LSPM J0859+2918 = NLTT 20681. Law et al (2008) derive a distance of     Law2008 
                       21.5 +10.1/-4.0 pc and a projected separation of 16.1 +8.2/-2.7 au.             
                       Estimated spectral types are M4.5 and M5.                                       
08596+0146 BAL1855     BAL2356a.                                                                       
08597-2749 TOK  23     Estimated period of visual pair 680y.                                   Tok2006 
                       A is SB2E, P=3.199d.  Tokovinin et al. (2006): dK(AB)=6.93,             Tok2006 
                       dJ(AB)=7.29 ==> M(B)=0.08 V(B)~18.5                                     Tok2014d
08599+0143 BAL1856     Previously known as BAL2356b.                                                   
08599-0135 HJ  111     HJL 102.                                                                HJL1986