3104C Remarks to table I and II. ----------------------------------------------------------- The following papers are referred to by number in Col. 5 of Table I and below: 00 Hoffleit (1982) 01 Houk and Cowley (1975) 02 Kennedy (1977) 03 Cowley (1976) 04 Harlan (1974) 05 Cowley and Fraquelli (1974) 06 Hube (1970) 07 Levato and Abt (1977) 08 Malaroda (1975) 09 Houk (1978) 10 Andersen and Nordstrom (1977) 11 Andersen and Nordstrom (1978) 12 Cowley and Bidelman (1979) 13 Houk (1982) ----------------------------------------------------------- HD Remark ----------------------------------------------------------- 256 Remark on spectrum in (10). 5042A Component A observed in very good seeing (sep. 0"9). 6530 Mass ratio: M2/M1= 0.88+0.24; remark on spectrum in (10). 9484 ESO spectra show no giant characteristics. 13936 Shell component in Ca II H and K lines (not sharp enough to be interstellar). 15004 Remark on spectrum in (10); Ca II K and Ti II 3759 double. 16701 Mass ratio: M2/M1= 0.88+0.11; remark on spectrum in (10). 17864 (06) gives RV= +17 (1plate). 18466 Mass ratio: M2/M1=0.91+0.11; Remark on spectrum in (10). 20606 (13) lists star as possibly composite. ESO spectra show normal late A spectrum with moderate rotation. 20888 Evans et al. (1964) give RV= +23 (4 plates). 21423 Possibly variable line width (maybe unresolved SB2). 24863A Remark on spectrum in (10). 31203 Listed as SB in Bright Star Cat. 31204 Fainter component of visual binary; brighter star is HD 31203, sep. 12". 31517 Abt (1970) gives RV= +11 (1 plate). 32846 Delta Scu variable X Cae; Bright Star Cat. gives RV= +6. 35859C Visual companion to HD 35860, sep. 38". 35860AB Mass ratio: M2/M1= 0.76+0.02; remark on spectrum in (10). 36058AB (06) gives RV= +25 (1 plate). 37306 Interstellar velocity: +17.3+4.4 (2 plates). 37594 Abt (1970) gives RV= +21 (1 plate). 38090 Remark on spectrum in (10). 38206 (06) gives RV= +25 (1 plate). 38616 Remark on spectrum in (10). 38735 SB3 and eclipsing variable V1031 Ori. Mass ratio: M2/M1= 0.97+0.32; full phot. and spect. analysis nearly completed. Remark on spectrum in (10). 39662A (06) gives RV= +28 (1 plate). Line profiles appear somewhat peculiar. 39789 Fairly broad shell-like component in Ca II K seen on two plates. 42536 Asymmetric H line profiles suggest traces of secondary spectrum. 42824 Weak interstellar Ca II K line. RV= +16.2+3.1 (2 plates). 45450 Mass ratio: M2/M1= 0.84+0.05; remark on spectrum in (10). 46730 Mass ratio: M2/M1= 1.01+0.21 ; remark on spectrum in (10). 48543A (13) lists spectral type as A3/5 + F/G; "spectrum overlapped with B component". 48797 (13) lists spectral type as A7/9 + F/G. 51210 Mass ratio indeterminate; remark on spectrum in (10). 52362 Mass ratio: M2/M1= 0.94+0.12; remark on spectrum in (10). 55595 Delta Scu variable (Baade & Stahl, 1982). 56455 Feinstein (1961) gives RV= +16 (1 plate). 58580 Mass ratio: M2/M1= 0.83:. (06) gives RV= +9 (1 plate). Lines very weak and difficult to measure; H lines omitted in mean. Definitive study requires higher S/N. Remark on spectrum in (10). 60168A Ellipsoidal variable RS Pup. Mass ratio: M2/M1= 0.47+0.09:. Remark on spectrum in (10). Possible indication of a third component on one plate, and of an interstellar Ca II K line on another (RV= +24+2). 61227 Beavers & Eitter (1981) give RV= +17.9+1.0. 62863 Eclipsing variable PV Pup. Full analysis by Vaz and Andersen (1984); mass ratio found here is M2/M1= 0.98+0.04. 63786 Mass ratio: M2/M1= 0.67+0.03; remark on spectrum in (10). 66255 Feinstein (1961) gives RV= +31 (1 plate). 69997 Delta Scu variable HQ Hya. 71581AB Eclipsing variable VV Pyx. Full analysis by Andersen et al. (1984a); some additional measurements of third component here. Mass ratio found here is M2/M1= 0.97+0.02. 74738 Fainter component of ADS 6988 (brighter comp. is Iota Cnc, HR 3475; sep. 30"). Bright Star Cat. gives RV= +16 (A) and +8 (B). 76270 Spectrum appears normal on ESO plates. 77640 Batten (1976) gives RV= +33.1+1.6 ( 7 plates) and lists spectrum as Ap. 79193 Eclipsing variable KM Hya. Full analysis by Andersen & Vaz (1984). 81009AB Variable Ap star KU Hya. 81471 Buscombe & Kennedy (1965) give RV= +28: (1 plate). 81728AB Shell star and also visual binary. Remark on spectrum in (10). 84984 Weak interstellar Ca II K line maesured on one plate; RV= +4+2. 85905 Remark on spectrum in (10). 86087 Mass ratio: M2/M1= 0.84+0.13; remark on spectrum in (10). 88195 Remark on spectrum in (10). 88699 Remark on spectrum in (11). 89911 Mass ratio: M2/M1= 0.93+0.02; remark on spectrum in (10). 93502A Mass ratio: M2/M1= 0.91+0.23; sharp lines, components approximately equal. 93903A Maybe not Am: Sc II Lines appear normal. Orbit by Worek et al. (1978). 99022 Remark on spectrum in (10). 99922A Remark on spectrum in (11). 103101A Spectral type by Hiltner et al. (1969) must be a misprint. 103516 Buscombe & Kennedy (1969) give RV= -21, Var. (1 plate). ESO plates cover too short time span for variability detection. 104035 Buscombe & Kennedy (1965) give RV= +2, Var. (2 plates). 105509 Eclipsing variable V788 Cen. Mass ratio: M2/M1= 0.56:. Remark on spectrum in (10). 106922AB Buscombe & Kennedy (1965) give RV= +6 (2 plates). 108925 Strong circum- or interstellar Ca II K line appears on two of the three plates. 111786 Lambda Boo star (10). (13) gives only spectral class A0 III, but Baschek et al. (1984) confirm the star as Lambda Boo type. 112074A Batten (1976) gives RV= -24.3+1.1 (5 plates). 114371A Mass ratio: M2/M1= 0.97+0.26; remark on spectrum in (10). 116458 Unusual Ap star; see remark in (01). 116836AB Possible weak double emission and sharp central absorption in H beta and H gamma. 120500 Batten (1976) gives RV= +9.4+2.0 var? (9 plates; HD no. misprinted as 120050). 123177 Batten (1976) gives RV= +10.5+2.2 (5 plates). 127208 Shell star, possible SB2; remark on spectrum in (10). 128974 Si II lines not particularly strong; He I and Mg II 4481 weak. He weak star? 133792 Buscombe & Kennedy (1969) give RV= +15 (1 plate). 135730 Buscombe & Kennedy (1965) give RV= -6, var. (2 plates). 136347A Kearsley & Wegner (1978) give RV= -53 (1 plate). 138488A Brighter component of ADS 9689; sep. 9". 138488BC Fainter component of ADS 9689. 139271A ESO plates show no obvious Am characteristics. 139518 Bright Star Cat. gives spectral class as B5 Ia, which must be a mistake. 142445 Neubauer (1930) gives RV= -5 (2 plates). 143248A Buscombe & Kennedy (1965) give RV= +11 (2 plates). 144667 Peculiar He-weak star; see Andersen et al. (1984b). 144668 Variable pre-main sequence star V856 Sco (see e.g. The & Tjin A Djie, 1979). Full spectroscopic analysis in progress. 147614A Line widths appear variable; possibly unresolved SB2. 147779 Variable comparison star used in study of V760 Sco. (Andersen et al., in prep.). Remark on spectrum in (11). 149886AB B component not visible on ESO spectra. 150026 Evans et al. (1964) give RV= +2 (5 plates). 150573 Bessell & Eggen (1972) quote RV= -17. 151566A Brighter component of visual binary; sep. 3"2. (09) gives combined spectral class F0 IV/V. 151566B Companion to preceding star; remark on spectrum in (10). 151676 Eclipsing binary V1010 Oph; sp. orbit by Guinan & Koch (1977). 152082A Remark on spectrum in (10) 154972 Evans et al. (1964) give RV= -8 (4 plates). 166469 Kearsley & Wegner (1978) give RV= -8 (1 plate). 168646 Remark on spectrum in (10). 169268 Mass ratio: M2/M1= 0.83+0.09; remark on spectrum in (10). 170030 Member of NGC 6633, see (07) and remark in (10) about HD 170054. Velocity found here agrees with cluster velocity as given by Petrie (1953). 174115 SB2 with very low amplitude: line widths vary. Components nearly equal. 178299 Mass ratio: M2/M1= 1.01+0.04; remark on spectrum in (10). 183552 Remark on spectrum in (10). 185404AB Only one spectrum visible on ESO plates. 188405AB Spectrum probably triple-lined; mass ratio cannot be determined from present radial velocity data. 191095AB Component 1 has constant velocity. Mass ratio M3/M2= 0.98+0.09; V0 as found from comp. 2 and 3 is -2.1+3.7. Remark on spectrum in (10). 199475 Delta Scuti variable EM Aqr. 199603 Eclipsing binary DV Aqr; sp. orbit by Paffhausen and Seggewiss (1976). 200496 Fainter component of visual binary; brighter component is HR 8059, sep. 2"7. 203548 Remark on spectrum in (11). 208496 Mass ratio: 0.85; primary component has somewhat stronger and broader lines than secondary. Also eclipsing binary (Manfroid & Mathys, 1984). 208612 Remark on spectrum in (10). 209278A Eclipsing binary DX Aqr. Sp. orbit by Paffhausen and Seggewiss (1976), who give V0= +15.0. Brighter component (photographically) of ADS 15562, sep. 3"6. ADS 15562 B has RV= 15.7+0.9 (Andersen and Nordstrom, 1983b). 220003A Remark on spectrum in (11). Jeffers et al. (1963) give sep. 0"5; observed sep. was 2" in 1975. 220392A Remark on spectrum in (01). 223884 Remark on spectrum in (10).