X-ray Statistics of WR Colliding-Wind Binaries

Details X-ray Statistics of WR Colliding-Wind Binaries X-ray Statistics of WR Colliding-Wind Binaries

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..404..212k&link_type=abstract

The Eighth Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conference Series, Vol. 404, proceed

Astronomy and Astrophysics

Astrophysics

Scientific paper

Statistical correltation between X-ray luminosity and orbital priod of WR + O binaries which are suspected to have strong colliding-wind activities is considered. Results show that short-period binaries have similar X-ray luminosity with single WR stars, while binary stars with long-period and high eccentricity can be strong X-ray emitter at some phase of orbital motion.

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