Estimation of steady-state basic parameters of stars

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dc.creatorVasiliev, B. V.
dc.date2000-03-29
dc.date2000-03-30
dc.date.accessioned2026-07-07T01:52:56Z
dc.date.available2026-07-07T01:52:56Z
dc.descriptionFrom a minimum of total energy of celestial bodies, their basic parameters are obtained. The steady-state values of the mass, radius, and temperature of stars and white dwarfs, as well as masses of pulsars are calculated. The luminosity and giromagnetic ratio of celestial bodies are estimated. All the obtained values are in a satisfactory agreement with observation data.
dc.description17 pages,4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0003432
dc.identifierhttp://arxiv.org/abs/astro-ph/0003432
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/792
dc.subjectAstrophysics
dc.titleEstimation of steady-state basic parameters of stars
dc.typetext

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