Velocity Fields at the Surface of ZZ Ceti Stars

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dc.creatorKoester, D.
dc.creatorKompa, E.
dc.date2007-02-02
dc.date.accessioned2026-07-07T07:44:23Z
dc.date.available2026-07-07T07:44:23Z
dc.descriptionWe demonstrate that the peculiar line profiles observed in DA white dwarfs in the temperature range of the ZZ Ceti variables can be explained by the surface velocity fields associated with the pulsations.
dc.description4 pages, 4 figures, to be published in the proceedings of the 15th European Workshop on White Dwarfs (ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0702067
dc.identifierhttp://arxiv.org/abs/astro-ph/0702067
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/123180
dc.subjectAstrophysics
dc.titleVelocity Fields at the Surface of ZZ Ceti Stars
dc.typetext

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