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X-ray properties of early-type binaries: theory versus observations

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Early-type binary stars are expected to be more luminous and hard X-ray sources than single stars are. However, recent observational studies show that, on average, the X-ray properties of single and binary early-type stars are not very different. We review these studies and discuss a possible explanation for this discrepancy.
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Keywords: Close binary stars; Hot stars; Stellar winds; X-ray properties;Wind-wind collision

Document Type: Research Article

Affiliations: Sternberg Astronomical Institute, Moscow University, Moscow, Russia

Publication date: 2007-02-01

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