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Table 1.

Stellar demographics of X-ray sources within Wd1.

Spectral Cluster X-ray
type population detected
O9-9.5 III 27 1
O9-9.5 II,II-III 12 1
O9-9.5 Iab,Ib 30 19
B0-0.5 Ia,Iab,Ib 23 6
B1-1.5 Ia,Iab 10 0
B2-4 Ia 7 0
B5-9 Ia+ 4 0
LBV 1 0
YHG+RSG 10 0
O4-8 Ia+ 2 2
B0-2Ia+/WNVL 4 2
sgB[e] 1 1
OB SB2 2 2
WN5-8 14 8
WC8-9 8 3

Notes. Summary of X-ray detections by spectral type. The top panel reflects the expected evolutionary pathway for single stars, the second the possible products of binary interaction and the third WRs – a structure chosen to reflect the discussion in Sect. 3. We note that the marginal X-ray detections discussed in Sect. 3.4 are not included here. The X-ray detections Wd1-13, W1033 and Wd1-232 are included with the B0-2Ia+/WNVL, O9-9.5 II-III and B0-0.5 Ia,Iab,Ib sub-sets, respectively. The OB2 SB2 grouping comprises the optically and X-ray luminous systems Wd1-36 and -53a. A further ten optically faint O+O binaries of uncertain spectral type and luminosity class are excluded from the table, as is the sole Be star; none of these are X-ray detections.

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