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Obscuring Supersoft X-ray Sources in Stellar Winds
Published online by Cambridge University Press: 17 January 2013
Abstract
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We investigate the possibility of obscuring supersoft X-ray sources in the winds of companion stars. We derive limits on the amount of circumstellar material needed to fully obscure a ‘canonical’ supersoft X-ray source in the Large Magellanic Cloud, as observed with the Chandra X-ray Observatory.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 140 - 144
- Copyright
- Copyright © International Astronomical Union 2013
References
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