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arXiv · 1109.5866

Obscuring Supersoft X-ray Sources in Stellar Winds

Mikkel Thomas Bøje Nielsen·Carsten Dominik·Gijs Nelemans
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Abstract

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.

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Mikkel Thomas Bøje Nielsen, Carsten Dominik, Gijs Nelemans. 2011-09-27. Obscuring Supersoft X-ray Sources in Stellar Winds. https://arxiv.org/abs/1109.5866

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