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Table D.2.

Parameters for WC stars in the LMC. Parameters of stars which are excluded from our analysis (see Sect. 4) are colored in gray.

BAT99 spectral subtype (a) MV(a) log(L) log(Llit) Binary? (a, b) P (c)
[mag] [L ] [L ] [d ]
9 WC4 -4.4 5.49 5.48 (d) - -
8 WC4 -4.2 5.41 5.42 (e) - -
10 WC4(+O9.5II:) -5.1 5.77 - ? -
11 WC4 -5.5 5.93 5.70 (e) - -
20 WC4+O -4.6 5.57 - - -
28 WC6+O5-6V-III(+O) -6.5 6.33 - x 14.926
34 WC4+OB -5.8 6.05 - ? -
38 WC4(+O8I:) -7.2 6.61 - x 3.0328
39 WC4+O6V-III(+O) -6.1 6.17 - x 1.9169
52 WC4 -4.5 5.53 5.65 (e) - -
53 WC4(+OB) -5.4 5.89 5.35 (f) ? -
61 WC4 -5.0 5.73 5.68 (e) - -
70 WC4(+OB) -5.3 5.85 - ? -
85 WC4(+OB) -7.7 6.81 - ? -
84 WC4(+OB) -5.4 5.89 - ? -
87 WC4+OB -4.8 5.65 - ? -
90 WC4 -4.6 5.57 5.44 (e) - -
115 WC4(+OB) -5.7 6.01 - ? -
101 WC4(+WN6+O) -7.5 6.73 - ? -
121 WC4 -4.7 5.61 - - -
125 WC4(+OB) -5.6 5.97 - ? -
127 WC4(+O) -6.2 6.21 - ? -

(a) Values adopted from Bartzakos et al. (2001a). (c) We mark a binary with an “x” if it is known as an SB1 or SB2 binary, if it shows indications of binarity (see table 6 in Bartzakos et al. (2001a)) it is marked with an “?”. (c) Values taken from Bartzakos et al. (2001b). (d)Calculated by Hillier et al. (2021). (e)Calculated by Crowther et al. (2002). (f) Calculated by Ramachandran et al. (2018).

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