XMM-Newton observation of the highly magnetised accreting pulsar Swift J045106.8-694803: evidence of a hot thermal excess
Several persistent, low luminosity (<i>L<sub>X</sub></i> ~ 10<sup>34</sup> erg s<sup>-1</sup>), long spin period (P > 100 s) High Mass X-ray Binaries have been reported with blackbody components with temperatures > 1 keV. These hot thermal excess...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
2013-11-16.
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| Subjects: | |
| Online Access: | Get fulltext |