4520A    Both components have very sharp lines of slightly unequal strength.
 13765     Low-amplitude SB2 according to CORAVEL observations.
 19330     Not Pop. II star (Nissen prog.).
 31623     HR 1591. Not Pop. II stars (Nissen prog.).
 38510     Very weak lines.
 39917     RS CVn-type binary SZ Pic (Andersen et al., 1980).
 42988     Double lined binary according to CORAVEL observations.
 43760     HR 2255. Not Pop. II star (Nissen prog.).
 51081     Photometric variable (Olsen, 1983A&AS...54...55O)
 57749     HR 2811. Not Pop. II star (Nissen prog.).
 66061     Composite spectrum (A0:nn + G0:III:).
 71433     HR 3325; variable velocity (Andersen et al., 1984). Not Pop. II star (Nissen prog.).
 72617     HR 3380. Not Pop. II star (Nissen prog.).
 84850     HR 3887. Not Pop. II star (Nissen prog.).
101614     Equal components, sharp lines.
105274     Low-amplitude SB2 according to CORAVEL observations.
128279     Extremely weak lines.
139941     Probably variable according to preliminary CORAVEL data.
149960     Probably variable according to preliminary CORAVEL data.
154107     Composite spectrum (A0-1:s + G0:III:).
170747     CaII H and K emission. Possibly photometric variable (Olsen, 1983A&AS...54...55O).
170899     Composite spectrum (A2:: + K2:III:).
172503     Reddened B8::nn; v sini approx. 250 km s. Interstellar CaII K-line velocity is -3km/s .
172914     Very weak lines.
174930     Probably variable according to preliminary CORAVEL data.
177352     Visual binary: sep. approx. 1", {delta}-m approx. 0.3. Also SB3
177352     Component 3 has sharp lines which may be those of the visual companion: RV=-4.9+/-2.7 (5 lines). 
177352     Line strengths and widths decrease in order 1:2:3. Quite weak lines.  
184266     Weak lines.  
187858AB   Low-amplitude SB2 according to CORAVEL observations.  
191365     SB2 according to CORAVEL observations.  
193565     Very weak lines; CORAVEL observations show probable variability.  
209837     Low-amplitude SB2 according to CORAVEL observations.  
210737     SB2 with almost equal components; see Sect. 6.