Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S281(7), p. 140-144, 2011
DOI: 10.1017/s1743921312014883
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Obscuring Supersoft X-ray Sources in Stellar Winds
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Abstract
AbstractWe 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.
