Radial solitary waves in periodic variable stars

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dc.creatorPrigara, Fedor V.
dc.date2006-08-29
dc.date2006-09-15
dc.date.accessioned2026-07-07T07:19:27Z
dc.date.available2026-07-07T07:19:27Z
dc.descriptionIt is shown that the oscillations of brightness in classical Cepheids and other 'pulsating' variable stars are caused rather by the passing of radial solitary waves through the photosphere of a star, than by pulsations of a star. Radial solitary waves also determine the oscillations of brightness in some other types of periodic variable stars ordinary not considered as pulsating stars.
dc.description5 pages, REVTeX, discussion of Beta Lyrae and UV Ceti stars added
dc.identifierhttps://arxiv.org/abs/astro-ph/0608622
dc.identifierhttp://arxiv.org/abs/astro-ph/0608622
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/114627
dc.subjectAstrophysics
dc.titleRadial solitary waves in periodic variable stars
dc.typetext

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