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Table B.1

Sources of spectroscopic data, line profile variation (LPV), and comments about binarity/multiplicity.

Star Medusa UVES ARGUS SINFONI HST/FOS HST/STIS HST/COS HST/GHRS IUE LPV Comments Source †
016 Xa – – – – – Xg – – no – 1 x
063 Xa – – – – – – – – yes SB2 1 –
064 Xa – – – – – – – – yes weak RV 1 x
072 Xa – – – – – – – – no – 1 x
094 Xa – – – – – – – – yes SB2 1 –
108 Xa – – – – – – – X no – 7 x
145 Xa – – – – – – – – yes weak RV, MULT 1 –
147 Xa – – – – – – – – yes? MULT 7 –
151 Xa – – – – – – – – yes weak RV, MULT 1 –
169 Xa – – – – – – – – no – 1 x
171 Xa – – – – – – – – yes weak RV 1 x
180 Xa – – – – – – – X yes weak RV 1 x
208 Xa – – – – – – – – no weak RV 1 –
216 Xa – – – – – – – – no – 1 x
259 Xa – – – – – – – – no weak RV 1 x
267 Xa – – – – – – – – ? weak RV 1 x
333 Xa – – – – – – – – yes weak RV 1 x
402 Xa – – – – – – – X yes SB2? 3, 4, 7 –
404 Xa – – – – – – – – no SB1 1 x
406 Xa – – – – – – – – no ASYM? 1 –
422 Xa – – – – – – – – ? SB1 1 x
427 Xa – – – – – – – – no – 4 x
440 Xa – – – – – – – – yes SB2? 1 –
445 Xa – – – – – – – – no SB2 1 –
455 Xa – – – – – – – – yes SB1, ASYM 1 x
457 Xa – – – – – – – – no? – 7 x
468 Xa – – – – – – – – no MULT 1 –
482 – Xa – Xb Xc Xd,e – – – yes? SB1, MULT? 3, 5 x
506 Xa – – – – – – – – yes weak RV 1 x
509 Xa – – – – – – – X yes SB2 3, 7 –
512 Xa – – – – – – – – yes SB1 1 x
518 Xa – – – – – – – – no weak RV 1 x
527 Xa – – – – – – – X yes SB2 1 –
532 Xa – – – – – – – – no SB1 1 x
538 Xa – – – – – – – – yes SB2 1 –
542 Xa – Xa Xb – – – – – yes SB1 2 x
545 – Xa Xa Xb – – – – – no weak RV 2 x
562 – Xa – – – – – – – ? ? – –
566 Xa – – – – – – – – no – 1 x
599 Xa – – – – – – – – no weak RV 1 x
603 Xa – – – – – – – – yes SB1 1 x
608 Xa – – – – – – – – yes SB1 1 x
617 Xa – – – – – – – X yes – 7 x
621 Xa – – – – – – – – no DBL 1 x
626 Xa – – – – – – – – no – 1 x
664 Xa – – – – – – – – no – 1 x
669 Xa – – – – – – – – no weak RV 1 x
682 Xa – – – – – – – – no – 6 x
695 Xa – – – – – – – X yes SB1 3, 4, 7 x
755 Xa – – – – – – – – no – 1 x
758 Xa – – – – – – – X no? – 7 x
797 Xa – – – – – – – – no – 1 x
1001 – – Xa Xb Xc – – – – no? – 2 x
1014 – – Xa – Xc – – – – no SB1 2 –
1017 – – Xa Xb Xc Xd – – – yes weak RV 2 x
1018 – – Xa Xb Xc – – – – no SB1 2 x
1021 – – Xa Xb Xc – – – – no weak RV 2 x
1022 – – Xa Xb Xc X e – – – no weak RV 2 x
1025 – – Xa Xb Xc – – – – yes MULT? 2 x
1026 – – Xa Xb Xc – – – – no SB1 2 –
1028 – – Xa Xb Xc – – – – no – 2 –
Mk42 – Xf – Xb – – – Xh – ? MULT? – x

Notes. Comments: single-lined (SB1), double-lined (SB2) spectroscopic binary, asymmetric profile (ASYM), and double (DBL) or multiple (MULT) sources in HST images. Sources: (1) Sana et al. (2013); (2) Hénault-Brunet et al. (2012); (3) Schnurr et al. (2008); (4) Doran et al. (2013); (5) Massey et al. (2005); (6) Bestenlehner et al. (2011); (7) this work. Observations:

(a)

program ID: 182.D-0222 (PI: Evans);

(b)

program ID: 084.D-0980 (PI: Gräfener);

(c)

program ID: 6417 (PI: Massey);

(d)

program ID: 7739 (PI: Massey);

(e)

program ID: 9412 (PI: Massey);

(f)

program ID: 70.D-0164 (PI: Crowther);

(g)

program ID: 11484 (PI: Hartig);

(h)

program ID: 3030 (PI: Ebbets).

(†)

Stars mark with x are considered in the discussion.

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