Table 3
Objects in our FORS 2 sample with available X-ray observations.
Object | Spectral | LX | Adopted | References | Comments |
type | distance | ||||
[1031 erg s-1] | [kpc] | ||||
|
|||||
BD −12° 4982 | B0 II | 1 | 1.5 | 1 | |
HD 110432 | B2 pe | 40 | 0.37 | 2, 3 | γ Cas-analog |
HD 120324 | B2 Vnpe | 0.06 | 0.115 | 4 | |
HD 120991 | B2 IIne | 30 | 0.83 | 4, 5 | γ Cas-analog? |
HD 164816 | O9.5 V + B0 V | 3 | 6 | 6 | X-ray pulsations |
HD 165052 | O7 Vz + O7.5 Vz | 300 | 1.2 | 7 | colliding wind binary |
HD 166033 | B1 V | 800 | 1.5 | 4, 8 | |
HD 315032 | B2 Vne | 10 | 1.2 | 9 | |
HD 345439 | B1/B2 V | <0.05 | 1.5 | 10 | σ Ori E-analog |
|
|||||
CPD -59° 2624 | O9.5 V | 1.9 | 2.3 | 11 | |
HD 37020 | B0.5 V | 25 | 0.45 | 12 | |
HD 46056 | O8 V | 32.5 | 1.4 | 13 | |
HD 46106 | O9.7 III | 0.9 | 1.4 | 13 | |
HD 46149 | O8.5 V((f)) | 1.1 | 1.4 | 13 | |
HD 46150 | O5 V((f)) | 22 | 1.4 | 13 | |
HD 46202 | O9 V((f)) | 1.3 | 1.4 | 13 | |
HD 46223 | O4 V((f)) | 24 | 1.4 | 13 | |
HD 46328 | B0.7 IV | 3 | 0.42 | 14 | X-ray pulsations |
HD 60848 | O8:V: | 0.13 | 0.5 | 15 | |
HD 93027 | O9.5 IV | 1.3 | 2.3 | 11 | |
HD 93521 | O9 Vp | 1.1 | 1.2 | 16 | |
HD 101008 | B1 II/III | 3 | 2.3 | 17 | |
HD 117357 | O9.5/B0 V | 20 | 7 | 18 | |
HD 125823 | B7 IIIpv | 0.005 | 0.14 | 19 | |
HD 152246 | O9 IV | 14 | 1.6 | 20 | triple |
Notes. Distances and the interstellar absorption column density – used to derive LX – are estimated on the basis of UBV photometry, or taken from the literature.
Reference. (1) De Becker et al. (2005); (2) Motch et al. (2015); (3) Torrejón et al. (2012); (4) Oskinova et al. (in prep.); (5) Frémat et al. (2002); (6) Trepl et al. (2012); (7) Pittard & Parkin (2010); (8) Dahm et al. (2012); (9) Damiani et al. (2004); (10) Eikenberry et al. (2014); (11) Nazé et al. (2011); (12) Stelzer et al. (2005); (13) Wang et al. (2008); (14) Oskinova et al. (2014); (15) Rauw et al. (2013); (16) Rauw et al. (2012); (17) Nazé et al. (2013); (18) Beer (1961); (19) Nazé et al. (2014); (20) Nasseri et al. (2014).
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