577 1D: ADS 1582AB, 8.5, 11.0v, separation 2.3" at 188" from the bright component D. C, 9.2v at 31" from A.
592 1D: ADS 1625AB, compound multiple.
595 1D: Binary with HR 596, q.v.
596 1D: 4.18 A2p, 5.21 Am, 933.05y, a = 4.0". Colors for combined light. Combined mag 3.82V.
603 1D: compound multiple with HR 604.
604 1D: BC 5.5 B8V, 6.3 A0V, 61.1y, a = 0.296". ADS 1630BC compound multiple with HR 603. Component D, 15v at 28". Possibly also compound multiple with
604 2D: BD+41d408 at 53'.
605 1D: AB 5.90 F8IV, 7.27 F9V, 288.0y, a = 1.256"; or 309.03y, a = 1.34". Other published periods have ranged from 247 to
605 2D: 925y. Combined mag, colors.
609 1D: Suspected occultation double.
610 1D: ADS 1634AB compound multiple. B, G5V; C at 83" optical.
627 1D: B, mag diff 6.9v at 5.6".
628 1D: compound multiple with HR 629.
629 1D: compound multiple with HR 628.
640 1D: Resolved by speckle interferometry 1983.93, separation 0.07".
1708 1D: AP 0.6 G5III, 1.1 G0III, separation 0.04", 0.285y, a = 0.054", masses 2.67 and 2.55 solar. Combined mag, colors. Capella is
1708 2D: first star for which an orbit was determined from interferometer measures, by Anderson at Mt. Wilson in 1920. Speckle
1708 3D: separation 0.040" 1981.24 and 1981.68; 0.055" 1982.16. compound multiple with component H, a close binary, 10.0 dM1, 13.7 dM5 separation 2" at
1708 4D: 723" from A, probably physical with A. Other components all faint and distant from A.
1712 1D: Component B doubtful, possibly the nebula. C 10.7V at 30".
1713 1D: AxBC, compound multiple. BC binary, 7.6 B8II, 7.6v separation 0.12". D, 15.4v at 44". BC also classified B5V+B5V. For B, vsini =<39k/s.
1726 1D: compound multiple.
1728 1D: Possible compound multiple with HR 1732.
1729 1D: B, 13.4v at 29". C, 12.1v at 42" and D, optical.
5851 1D: compound multiple with HR 5852. Combined mag and colors, 5.53V, +0.23(B-V), +0.10(U-B).
5852 1D: compound multiple with HR 5851.
5853 1D: Quintuple system of which E is brightest companion; B, 12.0V at 4"; others at 172" and 208".
5854 1D: SR? Amp. 0.2V. ADS 9765B, optical.
5856 1D: AB binary; C, 9.0 G0 at 51" fixed.
5860 1D: Separation 0.097".
5864 1D: AB, compound multiple.
5867 1D: B, 9.72V, +0.84(B-V), +0.68(U-B), K3V, compound multiple. C, 10.7v at 201". Also compound multiple with BD+15d2906 at 1642", itself a double, 8.4,
5867 2D: 10.5v separation 6".
5873 1D: Component B, K0V. Third component optical.
5887 1D: Components white and orange-red.
5898 1D: B, 10.5v at 1.08"; C, 9.1 at 45"; D, 8.7 at 48".
5900 1D: Binary.
5904 1D: compound multiple. Combined mag, color.
5906 1D: Suspected occultation double.
5915 1D: Binary.
5918 1D: Companion G8V, optical.
5920 1D: Companion F5V, optical.
5925 1D: Binary with HR 5926. mag and color for combined light, 4.585V, +0.09(B-V), +0.07(U-B).
5926 1D: Binary with HR 5925.
5930 1D: Suspected occultation double.
5933 1D: Companions optical?
5944 1D: Primary is SB, 3.4, 6.4v separation 0.0003"; third component, ADS 9862B, 12.2v at 50". vsini both A and B =<100k/s.
5944 2D: Component B, F4V, optical.
5947 1D: Component B, 12.6v at 2", compound multiple.
5948 1D: AB binary. Companion A5Vp.
5953 1D: Possible quadruple system: SB 3.0, 5.0v, separation 0.00001", 3.3v at 0.1", and 4.9v at 0.186".
5954 1D: Component B optical.
5958 1D: Visual companion doubtful.
5961 1D: AB 5.3 A5V, 5.5 A6V, 26.93y, a = 0.366". C, 7.5v at 11". Combined mag, colors.
5968 1D: Companion optical.
5977 1D: Binary with HR 5978, q.v.
5978 1D: Quintuple system ADS 9909A-C is compound multiple with ADS 9910, 7.4 G8V, 8.1K0V separation 11" at 281" from ADS 9909A. ADS 9909AB 4.9 F5IV,
7683 1D: B, 13.2v at 12", optical. C, 12.5v at 40".
7689 1D: AD compound multiple. B, 13.7v at 23"; C, 11.6v at 36".
7693 1D: Binary.
7703 1D: AB compound multiple. B, 11v dM5, separation 6.6". Wroclaw contr. no. 16 gives mag differences but no separation for four components: AB 5.4v,
7703 2D: AC 5.15, and AD 4.0. Possible misidentification? Discovered by John Herschel as simply double. Components C and D
7703 3D: apparently first listed by van Albada at Lembang in 1958; only magnitudes and no separations were indicated.
7705 1D: AB binary. B, 8.7v at 13". C, optical.
7717 1D: Discordance as to which component has the peculiar spectrum usually attributed to A. However, on the basis of better
7717 2D: spectrograms, Abt gives A = A0V, B = A0Vp(Sr,Cr st.,Ca wk.).
7723 1D: Binary.
7726 1D: AB compound multiple.
7730 1D: Component D of ADS 13554 of which primary is HR 7735.
7735 1D: Component C, 6.99V, -0.14(B-V), -0.58(U-B) B5V, vsini : 25k/s, at 107" fixed. AP probably single star.
7736 1D: B is K1III, optical, vsini =<54k/s.
7737 1D: AB and AC both binary. C, 9v at 12".
7739 1D: AB compound multiple, 680?y.
7743 1D: compound multiple.
7747 1D: See note for HR 7754. ADS 13632B, 14v at 44"; C, 9.6v K5III, at 45" physical, vsini =<54k/s. D, 14.3v at 29" from C.
7754 1D: IDS notes Alpha1 Cap = HR 7747 (ADS 13632, four components) as one of five components of Alpha2 Cap = HR
7754 2D: 7754 = ADS 13645. Hence, we have recorded n = 9 for both. ADS 13645AB optical; BC 11.2, 11.5v, separation 1.2" binary.
7764 1D: Component C, photometric spectral class A2IV, vsini 53k/s. Component B, 10.1V at 4.1". For component AB, Rakos and
7764 2D: Mermilliod give 6.93V, +0.28(B-V), +0.24(U-B). However, other sources give the following V magnitudes:
7764 3D: Comp. 1976 1978 1980 Preferred
7764 4D: Gronbech and Oblak Ruffener
7764 5D: Olsen
7764 6D: AB 6.635 6.610 6.608 6.61
7764 7D: C 7.724 7.706 7.72
7764 8D: Colors converted from the uvby system (Gronbech and Olsen) are AB +0.13(B-V), +0.185(U-B); C +0.165(B-V), +0.14(U-B).
7767 1D: AB binary. C, at 34", 11.11V, +0.19(B-V), -0.29(U-B), B7Vp:, vsini 340k/s. D at about 45", 11.17V, +0.19(B-V),