Pulsating White Dwarfs in Cataclysmic Variables: The Marriage of ZZ Cet and Dwarf Nova

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dc.creatorWarner, Brian
dc.creatorWoudt, Patrick A.
dc.date2003-10-02
dc.date.accessioned2026-07-07T02:09:57Z
dc.date.available2026-07-07T02:09:57Z
dc.descriptionThere are now four dwarf novae known with white dwarf primaries that show large amplitude non-radial oscillations of the kind seen in ZZ Cet stars. We compare the properties of these stars and point out that by the end of the Sloan Digital Sky Survey more than 30 should be known.
dc.description4 pages, 2 figures; to appear in `Variable Stars in the Local Group', eds. Don Kurtz and Karen Pollard
dc.identifierhttps://arxiv.org/abs/astro-ph/0310072
dc.identifierhttp://arxiv.org/abs/astro-ph/0310072
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6628
dc.subjectAstrophysics
dc.titlePulsating White Dwarfs in Cataclysmic Variables: The Marriage of ZZ Cet and Dwarf Nova
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