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Table 1

Galactic WC stars, not visually obscured (van der Hucht 2001).

WR Subtype1 Figure2 Remarks3 WR Subtype1 Figure2 Remarks3
4 WC5 B.1
5 WC6 B.2 75a WC9 - no spectra
7a WN4h/WC - no spectra 76 WC9d - no spectra
8 WN7/WCE B.3 binary WN+WC? 77 WC8+OB - binary
9 WC5+O7 - binary 79 WC7+O5-8 - binary
11 WC8+O7.5 - binary 80 WC9d B.27
13 WC7 B.4 81 WC9 B.28
14 WC7+? B.5 binary? no d.e.l. 86 WC7+B0I-III B.29 binary: pseudo fit5
15 WC6 B.6 88 WC9+? B.30 WN+WC or WN/WC96
17 WC5 B.7 90 WC7 B.31
19 WC4pd+O9.6 - binary 92 WC9 B.32
20a WN7:h/WC - now WN6ha+WN6ha4 93 WC7+O7-9 - binary
23 WC6 B.8 95 WC9d B.33
26 WN7/WCE B.9 96 WC9d - no spectra
27 WC6 B.10 98 WN8/WC7 B.34 now WN7/WC+O8-97: pseudo fit
30 WC6+O6-8 - binary 98a WC8-9vd+? - no spectra
30a WO4+O5-5.5 - binary 101 WC8 - no spectra
31c WC6+OB - binary 102 WO2 B.35
32 WC5+OB - binary 103 WC9d B.36
33 WC5 B.11 104 WC9d+B0.5V B.37 binary: pseudo fit5
38 WC4 B.12 binary? 106 WC9d B.38
38b WC7+OB - binary 107a WC6 - no spectra
39 WC7+OB B.13 binary: pseudo fit5 111 WC5 B.39
41 WC5+OB - binary 112 WC9d+OB - binary
42 WC7+O7V - binary 113 WC8d+O8-9IV B.40 binary: pseudo fit5
45 WC6 B.14 114 WC5 B.41
47c WC5 - no spectra 117 WC9d B.42
48 WC6+O9.5 - binary 118 WC9d - no spectra
48a WC9d - no spectra 119 WC9d B.43
48b WC8ed - no spectra 121 WC9d B.44
50 WC7+OB B.15 binary: pseudo fit5 125 WC7ed+O9III B.45 binary: pseudo fit5
52 WC4 B.16 126 WC5/WN B.46
53 WC8d B.17 132 WC6 B.47
56 WC7 B.18 135 WC8 B.48
57 WC8 B.19 137 WC7pd+O9 B.49 binary: pseudo fit5
58 WN4/WCE B.20 140 WC7pd+O4-5 - binary
59 WC9d+OB? B.21 binary? 142 WO2 B.50
60 WC8 B.22 143 WC4+Be B.51 binary: pseudo fit5
64 WC7 B.23 144 WC4 B.52
65 WC9d+OB? B.24 binary? 145 WN7/WCE B.53
68 WC7 B.25 146 WC6+O8 B.54 binary: pseudo fit5
69 WC9d+OB? B.26 binary? 150 WC5 B.55
70 WC9vd+B0I - binary 153ab WN6/WCE+O6I - binary
73 WC9d - no spectra 154 WC6 B.56

Notes. 

(1)

Classification from van der Hucht (2001).

(2)

Spectral fits, shown in the appendix.

(3)

Further comments to the individual stars are given in Sect. A.

(5)

Known binary fitted as if it were a single star (as discussed in Sect. 2).

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