Massive Stellar X-ray Sources in the Galactic Center
Abstract
We present results of a spectroscopic survey of bright near-infrared counterparts to X-ray point sources from a deep Chandra survey of the Galactic nuclear bulge. K-band spectroscopy has revealed 13 new Wolf-Rayet and O-supergiant counterparts to Chandra sources in the Galactic center (GC). Although they are systematically softer in X-rays than the general GC source population of accretion powered cataclysmic variables (CVs), their X-ray colors indicate a hard component consistent with emission from plasmas with E > 2 keV. Such hard X-ray emission is not ubiquitous among single Wolf-Rayet and O stars, but is common among Wolf-Rayet+OB binaries with colliding supersonic winds. Although we regard colliding-wind binary hypothesis as the most likely scenario, it remains possible that several of these objects are wind-accreting neutron stars or black holes in supergiant high-mass X-ray binaries, or extraordinary single stars emitting hard X-rays.
Additional Information
© 2010 Astronomical Society of the Pacific.Attached Files
Published - Mauerhan2010p13505Hot_And_Cool_Bridging_Gaps_In_Massive-Star_Evolution.pdf
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Additional details
- Eprint ID
- 23366
- Resolver ID
- CaltechAUTHORS:20110418-113759972
- Created
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2011-05-04Created from EPrint's datestamp field
- Updated
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2019-11-04Created from EPrint's last_modified field
- Series Name
- ASP Conference Series
- Series Volume or Issue Number
- 425