Obscuring Supersoft X-ray Sources in Stellar Winds
classification
🌌 astro-ph.HE
keywords
x-raysupersoftobscuringsourceswindsamountcanonicalchandra
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.