The angular velocity of the apsidal rotation in binary stars

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dc.creatorVasiliev, B. V.
dc.date2004-05-15
dc.date2004-05-19
dc.date.accessioned2026-07-07T02:13:13Z
dc.date.available2026-07-07T02:13:13Z
dc.descriptionThe 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.
dc.description9 pages,1 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0405297
dc.identifierhttp://arxiv.org/abs/astro-ph/0405297
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7736
dc.subjectAstrophysics
dc.titleThe angular velocity of the apsidal rotation in binary stars
dc.typetext

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