Accretion geometry in the persistent Be/X-ray binary RXJ0440.9+4431
The persistent Be/X-ray binary RXJ0440.9+4431 flared in 2010 and 2011 and has been followed by various X-ray facilities (Swift, RXTE, XMM-Newton, and INTEGRAL). We studied the source timing and spectral properties as a function of its X-ray luminosity to investigate the transition from normal to fla...
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| Autors principals: | , , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
EDP Sciences
2014-01-01
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| Col·lecció: | EPJ Web of Conferences |
| Accés en línia: | http://dx.doi.org/10.1051/epjconf/20136406002 |
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