Modeling He-rich subdwarfs through the Hot-Flasher scenario: First Results
Astrophysics
2008-08-27 v1
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.
Keywords
Cite
@article{arxiv.0711.0140,
title = {Modeling He-rich subdwarfs through the Hot-Flasher scenario: First Results},
author = {Marcelo M. Miller Bertolami and Leandro G. Althaus},
journal= {arXiv preprint arXiv:0711.0140},
year = {2008}
}
Comments
2 Pages, 1 Figure, 1 Table. Presented at the Third Conference in Hydrogen Deficient Stars, Tubingen, September, 2007