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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