| Issue |
A&A
Volume 576, April 2015
|
|
|---|---|---|
| Article Number | A108 | |
| Number of page(s) | 31 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201425004 | |
| Published online | 10 April 2015 | |
Online material
Appendix A: Tables
Table of sources included in the sample of HMXBs.
Parameters of the continuum.
FeKα parameters.
Appendix B: Spectral atlas
BeXB
 |
Fig. B.1
BeXBs data, model, model components and ratio data/model. The spectra are typically soft, with no Fe emission lines. |
| Open with DEXTER | |
SGXB
 |
Fig. B.2
SGXBs data, model, model components and ratio data/model. The spectra are characteristically affected by high absorption, with Fe fluorescent lines. |
| Open with DEXTER | |
 |
Fig. B.2
continued. |
| Open with DEXTER | |
SFXT
 |
Fig. B.3
SFXTs data, model, model components and ratio data/model. |
| Open with DEXTER | |
γ Cassiopeae-like
 |
Fig. B.4
γ Cass-like systems data, model, model components and ratio data/model. The data is usually fitted using thermal models, including Fe recombination lines. FeKα is also usually visible. |
| Open with DEXTER | |
HMGB
 |
Fig. B.5
HMGBs data, model, model components and ratio data/model. Soft spectra with no sign of Fe lines. |
| Open with DEXTER | |
Unclassified
 |
Fig. B.6
AX J1749.1-2733 data, model, model components, and ratio data/model. We have no references for the luminosity class of the optical star, although the high absorption we observed points to a supergiant companion. |
| Open with DEXTER | |
Peculiars
 |
Fig. B.7
Peculiar sources data, model, model components and ratio data/model. These sources can hardly be categorized in any of the described HMXBs standard groups. |
| Open with DEXTER | |
© ESO, 2015
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