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X-ray Nova Binary Systems

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Abstract

The physical properties of X-ray novae as close binary systems are analysed. Observational data in X-ray, UV, optical, IR and radio ranges are summarized. Modern theoretical considerations of the problem of X-ray novae, taking into account some new ideas and results, are described. Properties of optical stars in X-ray novae are analysed. Data about the masses of black holes in X-ray binary systems are summarized. Possible evolutionary links between WR stars in close binary systems and X-ray novae are analysed.

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Cherepashchuk, A. X-ray Nova Binary Systems. Space Science Reviews 93, 473–580 (2000). https://doi.org/10.1023/A:1026507625481

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