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26 April 2024
 
  » arxiv » astro-ph/0405297

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The angular velocity of the apsidal rotation in binary stars
B.V.Vasiliev ;
Date 15 May 2004
Subject astro-ph
AbstractThe shape of a rotating star consisting of equilibrium plasma is considered. The velocity of apsidal rotation of close binary stars (periastron rotation) which depends on the star shapes is calculated. The obtained estimations are in a good agreement with the observation data of the apsidal motion in binary systems.
Source arXiv, astro-ph/0405297
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