Buried Binaries: Supergiants Feeding X-ray Pulsars?

Details Buried Binaries: Supergiants Feeding X-ray Pulsars? Buried Binaries: Supergiants Feeding X-ray Pulsars?

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20510212h&link_type=abstract

American Astronomical Society Meeting 205, #102.12; Bulletin of the American Astronomical Society, Vol. 36, p.1513

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Scientific paper

An XMM observation of the shell-like Galactic radio source G24.3+0.0 has revealed a bright, 113-second X-ray pulsar coincident with a highly reddened star with R-K>15. The object has a K-magnitude of 6.55, and is also detected in the MSX survey at 20μ Jy. The X-ray source has an absorbing column density of nearly 1023cm-2 and is highly variable. We explore models for this source and discuss its relationship to a number of other recently discovered pulsars which show similar highly absorbed and luminous companions.
This work is supported in part under a grant from the NASA XMM Guest Observer Program.

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