HIP 110842 (DK Tuc) Visual binary. A= 6.9; B= 10.2. Sep. 2.1" (HIP, HIP 110842 Perryman et al., 1997, Cat. ) HIP 060786 (DN Cru) Secondary eclipse might be the primary. Eccentric system. HIP 114175 (DN Tuc) Period might be half the value given. Very short eclipses GSC 7915 0741 = CPD -38 7598. Might be an RRc-type star with half the period. HD 101131 = HIP 56726 in the open cluster IC 2944. Eccentric. Slight apsidal HD 101131 motion. Period for primary eclipse given. Studied as a HD 101131 non-eclipsing system by Gies et al. (2002ApJ...574..957G). HD 174110 = BD-10 4817. HIP 032758 (KT CMa) Wrong period suggested in the HIP catalogue. (9.480d) HIP 078526 (MP TrA) Eccentric system. Visual binary. A=8.5; B=8.6 Hp. HIP 078526 Sep. 0.1" (HIP, Perryman et al., 1997, Cat. ). HIP 080022 (NSV 07597) Visual binary. A=9.2; B=10.0 Hp. Sep. 0.6" (HIP, HIP 080022 Perryman et al., 1997, Cat. ) HD 151475 (NSV 07976) V magnitudes calibrated with GCPD data (Mermilliod et HD 151475 al., 1997A&AS..124..349M). ASAS-3 data contaminated by companion. GSC 7372 0122 (NSV 08117) Might be EA-type. HIP 004505 (NSV 15212) Might be EB-type. HIP 034775 (NSV 17376) Koen and Eyer (2002, Cat. ) give HIP 034775 per=0.8025d. HIP 069617 (NSV 20064) Might be EB-type. HIP 075994 (NSV 20311) Might be EA-type. Koen and Eyer (2002, HIP 075994 Cat. ) give per=0.5431d. HIP 078808 (NSV 20495) Visual triple. AB=6.8"; AC=10.5" (Worley and Douglass, HIP 078808 1997, Cat. ). HIP 079970 (NSV 20579) Eccentric binary. HIP 092943 (NSV 24630) Eccentric. Slight apsidal motion. Period for primary HIP 092943 eclipse given HIP 098034 (NSV 24931) Koen and Eyer (2002, Cat. ) give HIP 098034 per=1.34736d. HIP 102935 (NSV 25363) Handler (1999MNRAS.309L..19H) wrongly classified it as HIP 102935 a DSCT? with a 0.526d period. HIP 105915 (NSV 25590) Koen and Eyer (2002, Cat. ) give HIP 105915 per=0.57773d. HIP 021213 (RZ Cae) Visual binary. A=7.8; B=9.6. Sep.=3.1" (HIP, Perryman HIP 021213 et al., 1997, Cat. ). GSC 6569 3789 (SW Pyx) No period in the literature. HIP 050463 (V340 Vel) Visual binary. A=8.3; B=9.2 Hp. Sep.=0.3" (HIP, HIP 050463 Perryman et al., 1997, Cat. ). HIP 051355 (V349 Vel) Also an intrinsic variable? (ACV: or DSCT:). Binarity HIP 051355 may have caused problems with HIP photometry. Visual binary. HIP 051355 A=10.0; B=11.2 Hp. Sep. =1.1". HIP 080545 (V373 Nor) Eccentric system. HIP 039229 (V414 Pup) Synchronous rotation. ACV and EA period are the same. HIP 039229 ACV var. =0.05mag. HIP 041250 (V438 Pup) Very eccentric. Multiple system. A=6.9; a=8.0; B=7.0 HIP 041250 (Tokovinin, 1997, Cat. ). Sep. AB=0.45"; Aa=0.049" HIP 041250 (Hartkopf et al., 1996, Cat. ). Period discovered HIP 041250 by visual observations. HIP catalogue suggested 5.699d. HIP 064941 (V963 Cen) Very eccentric. 0.08mag. scatter at maximum: possible HIP 064941 RS-type. HIP 078919 (V1046 Sco) Eccentric. HIP 086163 (V1082 Sco) Very eccentric. Also possible ACYG-type. HIP 086509 (V2383 Oph) Koen and Eyer (2002, Cat. ) give HIP 086509 per=0.12555d. HIP 89404 (V4386 Sgr) Too few observations of minima II. Secondary minimum HIP 89404 might be the primary. HIP 026772 (WZ Pic) Koen and Eyer (2002, Cat. ) give HIP 026772 per=0.60835d.