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Table A.2

Multiplicity and spectral types of PACWBs.

# Usual ID Status Sp. type(s) P Ref.

1 HD 15558 B (T?) O5.5III(f) + O7V 442 d 1, 2
2 δOri A T (O9.5II + B0.5III) + B? 5.733 d/>100 yr 3, 4
3 σOri AB M O9.5V + B0.5V (+ OBs?) ? 5
4 15 Mon B O7V(f) + O9.5Vn 25.3 yr 6
5 WR 8 B WN7 + WC(?) 38 d, 115 d 7, 8
6 WR 11 B WC8 + O7.5 78.53 d 9, 10
7 WR 14 B? WC7 ? 11
8 CD–47 4551 U O5If 12
9 WR 21a B O3f/WN6ha + O4 32.673 d 13
10 HD 93129A B O2If + O3.5V? ? 14
11 HD 93250 B O4III + O4III >100 d 15
12 η Car B ? + ? 2022.7 d 16
13 WR 39 B? WC7 ? 17
14 WR 48 T (WC5 + O6-7V) + OI? 19.138 d/? 18, 19
15 HD 124314 B? O6V(n)((f)) ? 20, 21
16 HD 150136 T (O3-3.5V((f+)) + O5.5-6V((f))) + O6.5-7V((f)) 2.675 d/8,2 yr 22, 23, 24
17 HD 151804 U O8Iaf 12
18 WR 78 U WN7h 11
19 WR 79a B WN9ha + ? many years 25
20 HD 152623 T (O7V((f)) + OB?) + OB? 3.9 d/? 25
21 WR 89 B WN8h + OB ? 11
22 WR 90 U WC7 11
23 WR 98 B WN7/WC + O8-9 48.7 d 26
24 WR 98a B WC9 + OB? 565 d 27
25 WR 104 B WC9 + B0.5V 220 d 28
26 WR 105 U WN9h 11
27 9 Sgr B O3.5V((f+)) + O5V ~ 8.6 yr 29, 30
28 WR 112 B? WC9 + ? ? 31
29 HD 167971 T (O6-7V + O6-7V) + O8I 3.321 d/~ 20 yr 32, 33
30 HD 168112 B? O5.5III(f+) (+ OB?) >1 yr 34, 35
31 CEN 1a B O4 + ? ? 36
32 CEN 1b B O4 + ? ? 36
33 WR 125 B WC7 + O9III >15 yr, ~20−22 yr 37, 38
34 HD 190603 U B1.5Ia 12
35 WR 133 B WN5 + O9I 112.4 d 39
36 WR 137 B WC7 + O9V-III 13.05 yr 40
37 WR 140 B WC7 + O5 7.9 yr 41, 42
38 Cyg OB2 #5 Q (Ofpe/WN9 + O6−7Ia) + OB? + B0V 6.598 d/6.7 yr/>9000 yr 43, 44, 45
39 Cyg OB2 #9 B O5I + O6-7I 2.35 yr 46, 47, 48
40 Cyg OB2 #8A B O6If + O5.5III(f) 21.908 d 49
41 Cyg OB2-335 B O7V + O9V a few days(?) 50
42 WR 146 B (T?) WC6 + O8? many years ? 51, 52
43 WR 147 B WN8 + B0.5V many years ? 53

Notes. Meaning of the status symbols: B is for binary system; T for triple system; Q: for quadruple system; B? for suggested binary; T?: for suggested triple system; M for multiple with undetermined number of components; U for undetermined.

Reference.1)Garmany & Massey (1981); 2) De Becker et al. (2006a); 3) Harvey et al. (1987); 4) Harvin et al. (2002); 5) Drake (1990); 6) Gies et al. (1993); 7) Niemela (1991); 8) Marchenko et al. (1998); 9) Schmutz et al. (1997); 10) North et al. (2007); 11) van der Hucht (2001); 12) Benaglia (2010), and references therein; 13) Niemela et al. (2008); 14) Nelan et al. (2004); 15) Sana et al. (2011); 16) Damineli et al. (2008); 17) Chapman et al. (1999); 18) Hartkopf et al. (1999); 19) Hill et al. (2002); 20) Feast et al. (1955); 21) Worley & Douglass (1997); 22) Niemela & Gamen (2005); 23) Mahy et al. (2012); 24) Sana et al. (2013); 25) Mason et al. (1998); 26) Gamen & Niemela (2003); 27) Monnier et al. (1999); 28) Tuthill et al. (1999); 29) Rauw et al. (2005); 30) Rauw et al. (2012); 31) Marchenko et al. (2002); 32) Leitherer et al. (1987); 33) De Becker et al. (2012); 34) De Becker et al. (2004a); 35) Blomme et al. (2005); 36) Hoffmeister et al. (2008); 37) Dougherty & Williams (2000); 38) Cappa et al. (2004); 39) Underhill & Hill (1994); 40) Lefèvre et al. (2005); 41) Marchenko et al. (2003); 42) Fahed et al. (2011); 43) Rauw et al. (1999); 44) Kennedy et al. (2010); 45) Linder et al. (2009); 46) van Loo et al. (2008); 47) Nazé et al. (2010); 48) Blomme et al. (2013); 49) De Becker et al. (2004b); 50) Kiminki et al. (2008); 51) Setia Gunawan et al. (2000); 52) Dougherty et al. (2000); 53) Williams et al. (1997).

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