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Paper: X-ray Statistics of WR Colliding-Wind Binaries
Volume: 404, The Eighth Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam Ching Leung
Page: 212
Authors: Kogure, T.
Abstract: Statistical correlation 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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