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Close Binary Stars. VIII: Close Binary Star Systems in the Late Stages of Evolution

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Abstract

A review of close binary systems (CBSs) in the late stages of evolution is presented. High-mass and low-mass CBSs are described separately: WR+OB systems, “quiet” X-ray binaries, massive transient X-ray binaries with Be stars, X-ray novae and bursters, cataclysmic and symbiotic binaries. Luminous blue variables (LBV objects) and radio pulsars in binary systems are discussed. Black holes in binary stellar systems, methods for their search, and black hole masses in X-ray binary systems are described. A number of specific systems are analyzed. The mass distribution of relativistic objects, WR stars, and their CO cores in binary systems is described. The masses of stellar black holes and the possibility of testing the theories of gravity are discussed. Possible variations in the orbital periods of X-ray binaries due to enhanced quantum evaporation of black holes are presented.

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Cherepashchuk, A.M. Close Binary Stars. VIII: Close Binary Star Systems in the Late Stages of Evolution. Astron. Rep. 66 (Suppl 1), S567–S691 (2022). https://doi.org/10.1134/S1063772922130108

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