Obscuring Supersoft X-ray Sources in Stellar Winds
  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. 
Mikkel Thomas B{\o}je Nielsen, Carsten Dominik, Gijs Nelemans
astro-ph.HE