The physical approach to the hot star description

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dc.creatorVasiliev, B. V.
dc.date2008-02-12
dc.date2009-04-19
dc.date.accessioned2026-07-07T13:05:20Z
dc.date.available2026-07-07T13:05:20Z
dc.descriptionThe theoretical discription of a hot star interior is obtained. It explains the distribution of stars over their masses, mass-radius-temperature and mass-luminosity dependencies. The theory of the apsidal rotation of binary stars and the spectrum of solar oscillation is considered. All obrained theoretical predictions are in a good agreement with the known measurement data, which confirms the validity of this consideration.
dc.identifierhttps://arxiv.org/abs/0802.1581
dc.identifierhttp://arxiv.org/abs/0802.1581
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/227457
dc.subjectAstrophysics
dc.titleThe physical approach to the hot star description
dc.typetext

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