00134+2659 HR 40. VB (368y G0III) and SB (6d G7V) at 18". 00247-2709 GJ 2005, visual quadruple composed of M5-dwarfs, 0.27" and 0.05" at 00247-2709 1.07" from each other. Short estimated periods, but no orbits yet. 00316-6258 HR 126+127+125, Beta Tuc. 6 components. The inner quadruple contains 00316-6258 2 VBs (2.4" B9V and 44.7y A2V) at 27". The distant pair at 544" is 00316-6258 itself a 0.1" VB with a short, but yet unknown period. 00345-0433 HIP 2713. VB (1.9" G8II) and SB1 (81d G0V) at 19.5". 00364-4908 HIP 2888 = GJ 24AB. Two SBs (3.7d G3V and 22d K0V) at 329", CPM. 01078+4651 HIP 5303. Two SBs (1551d K0III and 4.6d F7V) at 8.8". 01137+2435 HR 360 = Phi Psc. Two SBs (20.4y K0III and 2d K0V) at 7.9". 01157-6852 HR 377 = Kap Tuc. Two VBs (857y F6IV and 86y K2V) at 318". The 01157-6852 sub-systems are counter-rotating, not co-planar. 01256+3133 HIP 6668. Visual triple made of the close pair AB (4.5", F9V) and a 01256+3133 C-component at 57" which is a 15d SB2 twin. 01409+4953 HIP 7841. VB (92y K0V) and SB (2.2d K0V) at 6". 01413+2545 HR 484. Two SBs (4.4d F2V and 1.4d K4V) at 10.6". Aab can have an 01413+2545 unseen tertiary because its orbit is precessing. 02084+2819 HIP 9971, two SBs (208d K0 and 88d G5) at 20.7", metal-poor. 02084+2819 The G5V secondary is fainter and bluer than the K0 primary, its mass 02084+2819 of 0.71M_sun is assumed to match the dwarf luminosity of the K0V 02084+2819 component. 02124+3018 HR 642 = 6 Tri. Two twin SB2s (14.7d G5III and 2.2d F6V) at 3.8". 02124+3018 The Aab has an interferometric orbit, its masses are estimated from 02124+3018 Hipparcos parallax. B is 1.25mag above the MS, young? 02470-0952 HD 17386, two VBs (0.3" F6V and 0.7" F8V) at 21". 03368+0035 HR 1099, two SBs (2.8d G5IV and 1152d K6V) at 8". 04078+6220 HR 1260. The visual component B (O9.5V) is a quadruple composed of 04078+6220 the eclipsing binary SZ Cam (2.7d) and another 2.8-d SB at 0.06". 04078+6220 The component A at 17.9" is itself a 10-d binary, the whole system 04078+6220 belongs to the cluster NGC 1502. 04226+2538 HR 1369B = Chi Tau. The visual secondary is a tight quadruple 04226+2538 composed of SB2 (17.6d G0V) and a close pair of K4V dwarfs with yet 04226+2538 unknown period, which we assume to be 10d here. Only the mass sum of 04226+2538 this pair is known, so equal masses of 0.7 M_sun and a provisional 04226+2538 period 10d are adopted. The viausl primary A at 19.4" may itself be 04226+2538 a close binary. 04325+1731 GG Tau, PMS quadruple (0.26" K6V and 0.93" M5 at 10.3"). A 196-y 04325+1731 orbit is computed for the bright pair AB. 04327+2553 UZ Tau is a PMS quadruple (VB 0.37" M3 and SB 19d M1.5 at 3.5"). 04356+1010 HR 1458 = 88 Tau. Six components. The inner quadruple is a 18y VB 04356+1010 composed of two SB2s (3.6d A6Vm and 7.9d G2V). The distant component 04356+1010 B at 70" it itself a 1350d SB1. 04518+1339 HIP 22607. The outer system is a 95y VB, with two SB2s (144d F5V and 04518+1339 497d K1V) as components. Member of the Hyades. The estimated 04518+1339 inclinations of Aab and Bab are 49 and 32 deg, the inclinantion of 04518+1339 the visual orbit is 51deg. 05017+2640 HIP 23395. VB (25y, F7V) and SB (186d, G5V) at 78". 05078+3024 HIP 23873 = RW Aur. PMS quadruple composed of an SB (2.8d, G5Ve) and 05078+3024 a VB (0.12") at 1.4". Strong accretion and outflow. 05079+0830 HR 1664. Two VBs (200y A5m and 2.8") forming a wide CPM pair at 343". 05079+0830 An SB sub-system in A is suspected, ibut gnored here. 05098+2802 HR 1670. SB (33d, A5m) and VB (32y, dG7) at 11.6". 05168+4559 HR 1708, Capella. The 104d visual-interferometric pair of giants and 05168+4559 a 388y VB of M-dwarfs at 723" from each other. 05239-0052 HR 1782. SB (22.6d F%V) and VB (48y F8V) at 2.7". 05287-6527 HIP 25647. 17.6-yr astrometric binary Aab and 0.06" pair of M-dwarfs 05287-6527 Bab at 9". 05293+2509 HR 1821 = 118 Tau. Two VBs (1.8" B8.5V and 1" A2?) at 4.7", 05293+2509 discovered in 2005 with adaptive optics. 05320-0018 HR 1852 = Delta Ori. A VB (0.26" O9II, where primary is a 5.7d SB) 05320-0018 and another 26d SB (B2V) at 52". 05331-0143 HR 1863. Two visual pairs AB (1.6" B4V) and CD (0.7" B8) at 29.4". 05331-0143 The spectroscopic sub-system in A is ignored, no orbit yet. 06003-3103 HIP 28442 = GJ 225.2. Quadruple composed of two VBs (67.7y K5V and 06003-3103 24y K5V) at 4" from each other. Likely old and metal-poor. 06024+0939 HR 2124 = Mu Ori. A 18.8y VB where each component is an SB (4.4d A2V 06024+0939 and 4.8d F3V). A member of Hyades?? 06298-5014 HR 2384. Two VBs (53y F2V and 101y K-dwarfs) at 12". The two pairs 06298-5014 counter-rotate, not coplanar. 06504-3142 HR 2545. SB (28.6d B6V) and VB (0.6" A3) at 43". 06580+0218 HIP 33513. Two SBs (6.8d A7V and 4.5d F5V) in a tight 0.9" VB. 07184-5721 HIP 35374. Two VBs (0.26" G0V and 0.3" M1V?) at 2.4". This is a 07184-5721 perplexing case: while the faint BC binary was discovered by 07184-5721 Rossitter as early as 1930, the apparently easier system Aab was not 07184-5721 seen, revealed only by Hipparcos. 07346+3153 HR 2891 = Alpha Gem. The inner quadruple is a 445y VB composed of two 07346+3153 SB1s (9.2d A1V and 2.9d A2Vm). The faint companion C at 72" is a 07346+3153 0.8d EB YY Gem composed of twin M0V dwarfs. 08119-4844 HD 68826 = AO Vel. Eclipsing pair (1.6d B9p) and SB2 (4.1d A0?) in a 08119-4844 41-yr orbit around each other. 08211+4725 HIP 40925. Two VBs (1.7" F7V and 280y G7V) at 39". 08263-3904 HR 3327 = NO Pup. EB (1.26d B9V) and VB (0.1" A3V) at 8.1". 08269+3212 HD 71149. SB1 (1496d G4) and VB (123y K2) at 108". 08285-0231 HR 3337. VB (55y) composed of two SBs (2.5d A5m and 6d A5m). 08285-0231 Estimated inclinations of the SBs are 86 and 45 deg, the inclination 08285-0231 of the visual orbit is 84 deg. There is also a faint CPM component 08285-0231 at 18". 08468+0625 HR 3482 = Eps Hya. Pairs AB (15y G5III) and Cab (9.9d dF7) compose a 08468+0625 990-y VB, with an additional distant companion at 19". 08592+4803 HR 3569 = Iot UMa. VB (817y) composed of an SB (11y A7V) and another 08592+4803 VB (BC, 39.7y dM1). The outer and inner pairs counter-rotate. 09123+1459 HR 3650 = Pi Cnc. VB (984d G9V) and a 0.53" pair of L8 brown dwarfs 09123+1459 at 43", CPM. 10017+1725 HIP 49136 = XY Leo. Two SBs (0.28d K0V and 0.80d M1V) in a 19.6-y 10017+1725 orbit around each other. 10444-6000 HIP 52526 = QZ Car. Two SBs (20.7d O9I and 6d O9V) orbiting each 10444-6000 other with P=50y. Belongs to the cluster Collinder 228. 11029+3025 HIP 54003 = VW LMi. Two SBs (0.48d F3V and 7.9d G2V?) on a 355-d 11029+3025 orbit, the shortest outer period known for a quadruple. Estimated 11029+3025 inclinations of the SBs and the outer orbit are 90 and 39 deg, 11029+3025 57 deg. respectively. T.Pribulla (priv. comm.) found a CPM 11029+3025 companion, HD 95606=HIP 53969 at 340". It is not clear if this 11029+3025 companion is bound. 11037+6145 HR 4301 = Alp UMa. VB (44.5y K0III) and SB1 (6.0d F8) at 280". The 11037+6145 SB1 can have additional distant companion, as inferred from the 11037+6145 precession of its orbit. 11182+3131 HR 4375 = Xi UMa. Aab (1.83y G0V) and Bab (4d G5V) on a 60-y outer 11182+3131 orbit. The orbits of Aab and AB are close to coplanarity. A close 11182+3131 visual companion to B was discovered by speckle, but it is ruled out 11182+3131 by further observations and the long-term radial velocity coverage 11182+3131 of Bab which follows the outer orbit without any perturbations. 11221-2447 HIP 55505 = HD 98800. A young quadruple consisting of two SBs 11221-2447 (Aab 262d K4V and Bab 315d K7V?) on a 354y preliminary visual orbit. 11221-2447 The SB2 pair Bab was resolved interferometrically, it has a massive 11221-2447 circum-binary disk. 11395-6524 HR 4492 = GT Mus. SB1 (61d G2III) and EB (56d A0V) in a 0.22" VB with 11395-6524 yet unknown orbit. The mass of the secondary in the eclipsing 11395-6524 system is not known. 11480+2014 HR 4527 = 93 Leo. SB2 resolved interferometrically (71.7d A7V) and 11480+2014 SB1 (110y G5V) at 74", CPM. 12413-1301 HR 4822 = VV Crv. Two SBs (44.4d F5V and 1.5d F3V) at 5.3" from each 12413-1301 other, with a 5th component at 58.5". 13240+5456 HR 5054 = Zet UMa. Two SBs (20.5d A1Vp and 176d A7m) at 14.4", with a 13240+5456 5th companion at 709". 13461+0507 HIP 67186 = HT Vir. SB1(32d F8V) and EB (0.4d G0V) in 261y VB orbit 13461+0507 with inclination 43deg. 13532-3156 HR 5221 = 4 Cen. Two SB1s (6.9d B4IV) and (4.8d A3Vm) at 14.9". 14182-2731 HIP 69894. Two VBs (0.7" F7V and 0.4") at 3". 14593+4649 HIP 73346 = ET Boo. EB (0.65d F7V) and SB2 (31.5d G5V?) on a 67y VB 14593+4649 orbit with inclination 67deg. The estimated inclination of Bab is 14593+4649 58deg. 15118+6151 HIP 74370. Two similar EBs BV and BW Dra (0.35d F9V and 0.29d G3V) 15118+6151 at 16". 15122-1948 HR 5652 = Iot Lib. Two VBs (23.5y A0p) and (1.9" G8V?) at 57.8", CPM. 15245+3722 HR 5733 = Mu Boo. Two VBs (3.8y F1V and 257y G0V) at 109". The orbits 15245+3722 of the VBs are approximately co-planar. 15420+0027 HIP 76892. Two SBs (10.9d A5m and 15.8d A5m) on a 54y VB orbit. 15440+2220 HIP 77045. EB (15.9d F8) and SB1 (13.6d F8) in a 0.4" VB. 16058+1041 HIP 78864 = NQ Ser. Two SBs (4.3d G8IV EB and 11d K2V?) in a 0.23" 16058+1041 VB, with a faint CPM companion at 226" 16368+6948 HIP 81332. Two VBs (206y F5 and 0.6" F0) in a wide 147" CPM pair. 17116+3915 HIP 84100. Two VBs (0.4" F8 and 1.2" F8?) at 15", CPM. 17146+1424 HR 6406 = Alp Her. Close VB (Aab, 0.2" M5I) and SB1 (51.6d G5III) at 17146+1424 4.7". The mass of Ab is unknown, 7.5 M_sun assumed. A premature 17146+1424 3600y outer orbit is computed. 17465+2744 HR 6623. Astrometric binary (65y G5IV) and VB (43y M3) at 34". The 17465+2744 two inner orbits appear co-planar. 18002+8000 HR 6810 = 41+40 Dra. Two SB2s (Aab 1246d F7V and Bab 10.5d F7V) at 18002+8000 19" from each other. The Aab system has high eccentricity e=0.9754, 18002+8000 its visual orbit is known, it is not co-planar with the outer orbit. 18240+5848 HR 6923 = 39 Dra. The VB (6.6" A1V) and SB1 (2.7d F8V) are at 89" 18240+5848 distance, CPM. 18443+3938 HR 7051 = Eps Lyr. Two VBs (AB 1804y A4V and CD 585y A8Vn) at 209" 18443+3938 from each other. The inner orbits appear co-planar, but their 18443+3938 elements are still poorly defined owing to the long periods. The 18443+3938 component C was resolved interferometrically into a 0.19" pair, but 18443+3938 the reality of this sub-system is questionable. 18455+0530 HR 7048. Two VBs (51y or 27y A1V and 100y A1V) at 2.6", in a 18455+0530 configuration similar to Eps Lyr. The inner orbits are likely 18455+0530 co-planar. 19465+3343 HR 7534 = 17 Cyg. Two VBs (26" F7V and 232y K3V) at 792", CPM. 20194+1422 HIP 100192. SB1 (1092d) and VB (0.2" F5?) at 3.3". 20432+5707 HR 7940. SB2+EB (100d B2III) and SB1 (159d B2V?) in a tight 21y orbit 20587-7025 HIP 103545 = KZ Pav. EB (0.95d F6V) and VB (0.89" F9V?) at 7". 21424+4105 HR 8300 = 77 Cyg. Sextuple. The inner quadruple is a 27y pair AB 21424+4105 composed of two SBs (1.7d A1V and 35d B8V). There is also a CPM pair 21424+4105 with 109y period at 156" from AB. 23019+4220 HR 8762 = Omi And. VB (8.3y B6III) and SB2 (33d A2p) on a 68y outer 23019+4220 orbit. The inner and outer visual orbits are not co-planar. 23194-0507 HR 8868 = 96 Aqr. Two SBs (21d F3IV and 658d M0?) at 9.8". 23304+3050 HIP 116017. The quadruple is composed of two SB2s (1.9d F6V and 13d 23304+3050 F7V) on 48y orbit. There is a companion at 19".