Table 1
Spectral classifications, distances, and common aliases.
Name | HMXB type | Spectral type | Reference | Distance (a) | Alias names |
---|---|---|---|---|---|
of donor | (kpc) | ||||
HD 153919 | Persistent | O6 Iafpe | 1 | ![]() |
4U 1700-37, V* V884 Sco |
BD+60 73 | Intermediate | BN0.7 Ib | 2 | ![]() |
IGR J00370+6122 |
LM Vel | SFXT | O8.5 Ib-II(f)p | 3 | ![]() |
HD 74194, IGR J08408-4503 |
HD 306414 | SFXT | B0.5 Ia | 4 | ![]() |
IGR J11215-5952 |
BD+53 2790 | Persistent / Oe X-ray | O9.5 Vep | 5 | ![]() |
4U 2206+54 |
HD 100199 | Be X-ray | B0 IIIne | 6 | ![]() |
IGR J11305-6256 |
Notes. (a) The distances are adopted from Bailer-Jones et al. (2018). These distances are based on the Gaia DR2 measurements (Gaia Collaboration 2018) and were calculated by means of a Bayesian approach assuming an exponentially decreasing space density with the distance.
References. (1) Sota et al. (2014); (2) González-Galán et al. (2014); (3) Sota et al. (2014); (4) Lorenzo et al. (2014); (5) Blay et al. (2006); (6) Garrison et al. (1977).
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