A low luminosity state in the massive X-ray binary SAX J0635+0533

The X-ray pulsar SAX J0635+0533 was repeatedly observed with the XMM-Newton satellite in 2003-2004. The precise localization provided by these observations confirms the association of SAX J0635+0533 with a Be star. The source was found, for the first time, in a low intensity state, a factor ~30 lowe...

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Bibliographic Details
Published in:arXiv.org 2009-06
Main Authors: Mereghetti, Sandro, Nicola La Palombara
Format: Article
Language:English
Subjects:
Deposition
Luminosity
Pulsars
X ray binaries
X ray stars
XMM (spacecraft)
Online Access:Get full text
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Summary:The X-ray pulsar SAX J0635+0533 was repeatedly observed with the XMM-Newton satellite in 2003-2004. The precise localization provided by these observations confirms the association of SAX J0635+0533 with a Be star. The source was found, for the first time, in a low intensity state, a factor ~30 lower than that seen in all previous observations. The spectrum, well fitted by an absorbed power law with photon index ~1.7 and N_H = 1.2x10^22 cm^-2, was compatible with that of the high state. The low flux did not allow the detection of the pulsations at 33.8 ms seen BeppoSAX and RXTE data. In view of the small luminosity observed in 2003-2004, we reconsider the peculiarities of this source in both the accretion and rotation powered scenarios.
ISSN:2331-8422
DOI:10.48550/arxiv.0906.1685