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arXiv:astro-ph/0403117 (astro-ph)
[Submitted on 4 Mar 2004]

Title:The crust cooling curve of the neutron star in MXB 1659-29

Authors:Rudy Wijnands
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Abstract: We have monitored the quasi-persistent neutron-star X-ray transient MXB 1659-29 in quiescence using Chandra. The purpose of our observations was to monitor the quiescent behavior of the source after its last prolonged outburst episode and to study the cooling curve of the neutron star in this system. We discuss the results obtained and how they constrain the properties of the neutron star in MXB 1659-29
Comments: To appear in Proceedings of IAU Colloquium 194 "Compact binaries in the Galaxy and beyond" (Rev. Mex. A&A Conf. Series), eds. G. Tovmassian and E. Sion
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/0403117
  (or arXiv:astro-ph/0403117v1 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/0403117

Submission history

From: Rudy Wijnands [view email]
[v1] Thu, 4 Mar 2004 11:27:17 UTC (43 KB)
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