The apsidal motion in close binary stars

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dc.creatorVasiliev, B. V.
dc.date2001-10-10
dc.date.accessioned2026-07-07T02:00:47Z
dc.date.available2026-07-07T02:00:47Z
dc.descriptionIt is usually accepted to consider an apsidal motion in binary stars as a direct confirmation that a substance inside stars is not uniformly distributed. It is shown in this paper that the apsidal motion in binary systems observation data is in a good agreement with an existence of uniform plasma cores inside stars if they consist of hydrogen-deuterium-helium mixture.
dc.description9 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0110255
dc.identifierhttp://arxiv.org/abs/astro-ph/0110255
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3522
dc.subjectAstrophysics
dc.titleThe apsidal motion in close binary stars
dc.typetext

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