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Table 6.

Candidate binaries in Wd1.

ID Spectral type (a) Radial velocity X-ray (b) Infra red Radio Morphology
W9 sgB[e] (c) ° (c)
W15 O9 Ib ° ° (d)
W17 O9 Iab ° ° (d)
W27 O7–8 Ia+ °
W47 O9.5 Iab ° °
W65 O9 Ib ° ° °
W1001 O + O? °
W1002 O9 II–III + O?
W1006 O9–9.5 III bin? °
W1013 O + O? °
W1017 O9–9.5 III bin? °
W1018 O9.5 Iab °
W1026 O9–9.5 III
W1027 O9.5 Iab + O9 I–II? ° °
W1028 O9–9.5 III bin? °
W1029 O9–9.5 III bin? °
W1031 O9 III ° ° (e)
W1033 O9–9.5 I–III ° °
W1040 O9–9.5 I–III ° °
W1041 O9.5 Iab + ? ° °
W1042 O9.5 II
W1043 O9.5 II–III °
W1046 O + O? (g)
W1047 O9.5 II
W1055 B0 Ib + O? ° °
W1061 O9–9.5 III bin? °
W1066 O9 III
WR C WC9d (f)
WR H WC9d (f)
WR M WC9d + O? (f)
WR N WC9d ° (f) °
WR T WC9d (f)
WR U WN6o

Notes. Indicators of binarity are listed as RV changes, X-ray luminosity, an infra red excess, non-thermal radio emission, and spectral morphology (e.g. double lines, broad lines, or anomalously weak lines). Indicators that are strongly inconsistent with a single star are shown as solid circles, while indicators that suggest a binary interpretation are shown as open circles. Objects are listed if they (a) display substantial RV changes (ΔRV > 25 km s−1), (b) display any secondary indicator that is strongly inconsistent with a single star, or (c) display two or more indicators that individually suggest binarity.

References. (a)Clark et al. (2020), (b)Paper II, (c)Clark et al. (2013), (d)Dougherty et al. (2010), (e)Andrews et al. (2019), (f)Crowther et al. (2006), (g)Paper III.

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