White dwarf cooling by means of heat waves

dc.creatorFalcón Veloz, Nelson Leonardo
dc.date.accessioned2015-06-25T14:59:57Z
dc.date.accessioned2022-12-14T14:17:11Z
dc.date.available2015-06-25T14:59:57Z
dc.date.available2022-12-14T14:17:11Z
dc.date.created2015-06-25T14:59:57Z
dc.date.issued2005-06
dc.identifier14th European Workshop on White Dwarfs, ASP Conference Series, Vol. 334 Proceedings of a meeting held at Kiel, July 19-23, 2004. Edited by D. Koester and S. Moehler. San Francisco: Astronomical Society of the Pacific, 2005, p.69
dc.identifier1-58381-190-7
dc.identifierhttp://hdl.handle.net/123456789/1761
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5349441
dc.description.abstractThe standard white dwarf (WD) cooling theory is revised when the heat flux is propagate by thermal waves in degenerate material. Before the relaxation time, the luminosity function is dampening oscillation and the WD-age increase.
dc.languagees_ES
dc.publisherASP Astronomical Society of the Pacific
dc.relationVolumen 334, 2005;
dc.subjectDwarf cooling
dc.subjectThermal waves
dc.subjectDegenerate material
dc.subjectLuminosity function
dc.subjectDampening oscillation
dc.titleWhite dwarf cooling by means of heat waves
dc.typeArticle


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