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arXiv · 0711.0140

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

Marcelo M. Miller Bertolami·Leandro G. Althaus
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Abstract

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.

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Marcelo M. Miller Bertolami, Leandro G. Althaus. 2007-11-01. Modeling He-rich subdwarfs through the Hot-Flasher scenario: First Results. https://arxiv.org/abs/0711.0140

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