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Obscuring Supersoft X-ray Sources in Stellar Winds

Published online by Cambridge University Press:  17 January 2013

Mikkel T. B. Nielsen
Affiliation:
Department of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands email: m.nielsen@astro.ru.nl
Carsten Dominik
Affiliation:
Department of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands email: m.nielsen@astro.ru.nl Sterrenkundig Instituut “Anton Pannekoek”, Science Park 904, 1098 XH, Amsterdam, The Netherlands
Gijs Nelemans
Affiliation:
Department of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands email: m.nielsen@astro.ru.nl
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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
Copyright
Copyright © International Astronomical Union 2013

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