A convective model for light curves of ZZ Ceti Stars

dc.creatorFalcón Veloz, Nelson Leonardo
dc.date.accessioned2015-06-25T18:35:29Z
dc.date.accessioned2022-12-14T14:17:11Z
dc.date.available2015-06-25T18:35:29Z
dc.date.available2022-12-14T14:17:11Z
dc.date.created2015-06-25T18:35:29Z
dc.date.issued2005-06
dc.identifier14th European Workshop on White Dwarfs ASP Conference Series, Vol. 334, 2005
dc.identifier1-58381-190-7
dc.identifierhttp://hdl.handle.net/123456789/1765
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5349444
dc.description.abstractThe erratic behavior of the luminosity in ZZ Ceti light curves may be explained in terms of the sum of several convective fluctuations, where the heat flux is propagated in time by thermal waves. We present simulations of the light curves of GD29-38, GD 358, and HL Tau-76.
dc.languagees_ES
dc.publisherASP Astronomical Society of the Pacific
dc.relationVolumen 334, 2005;;
dc.subjectZZ Ceti
dc.subjectSeveral convective fluctuations
dc.subjectGD29-38
dc.subjectGD 358
dc.subjectHL Tau-76
dc.titleA convective model for light curves of ZZ Ceti Stars
dc.typeArticle


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