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Close Binary Stars. III: Roche Model

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Abstract

The article considers the Roche model as applied to close binary systems. The dimensionless potential of a system of two stars revolving around a common center of mass is presented. Modern methods for the synthesis of light curves and radial velocity curves of close binary systems (including X-ray systems) and their practical implementation are outlined, and solutions to model problems are presented. The synthesis of line profiles of optical stars in X-ray binaries is considered.

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    A. M. Cherepashchuk

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Cherepashchuk, A.M. Close Binary Stars. III: Roche Model. Astron. Rep. 66 (Suppl 1), S123–S167 (2022). https://doi.org/10.1134/S1063772922130054

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