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

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We 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.
2 Pages, 1 Figure, 1 Table. Presented at the Third Conference in Hydrogen Deficient Stars, Tubingen, September, 2007

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/167680

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0711.0140
 http://arxiv.org/abs/0711.0140
 Hydrogen-Deficient Stars ASP Conference Series, Vol. 391, proceedings of the conference held 17-21 September, 2007, p.265

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arXiv