Obscuring Supersoft X-ray Sources in Stellar Winds

Details Obscuring Supersoft X-ray Sources in Stellar Winds Obscuring Supersoft X-ray Sources in Stellar Winds

2011-09-27

arxiv.org/abs/1109.5866v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

Conference proceedings for IAU Symposium no. 281 "Binary Paths to Type Ia Supernova Explosions", 5-10 July 2011, Padova, Italy

Scientific paper

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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