Modeling He-rich subdwarfs through the Hot-Flasher scenario: First Results

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dc.creatorBertolami, Marcelo M. Miller
dc.creatorAlthaus, Leandro G.
dc.date2007-11-01
dc.date.accessioned2026-07-07T09:58:20Z
dc.date.available2026-07-07T09:58:20Z
dc.descriptionWe present first results from evolutionary simulations aimed at exploring the Hot-Flasher scenario for the formation of H-deficient subdwarf stars. The two types of late hot flashers that lead to He-enriched surfaces, "deep" and "shallow" mixing cases, are investigated for different metallicities.
dc.description2 Pages, 1 Figure, 1 Table. Presented at the Third Conference in Hydrogen Deficient Stars, Tubingen, September, 2007
dc.identifierhttps://arxiv.org/abs/0711.0140
dc.identifierhttp://arxiv.org/abs/0711.0140
dc.identifierHydrogen-Deficient Stars ASP Conference Series, Vol. 391, proceedings of the conference held 17-21 September, 2007, p.265
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/167680
dc.subjectAstrophysics
dc.titleModeling He-rich subdwarfs through the Hot-Flasher scenario: First Results
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