The Determination of a Radius of a Star Satellite in the Detached and Semidetached Close Binary System

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

For detached and semi-detached close binary systems a formula is derived
determining the radius of a star-satellite in terms of stellar mass of
the components and the distance between them. The test of the formula
has been made according to data of Svechnikov's and Bessonova's
Catalogue and a good result has been obtained.

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