The Formation of Hydrogen Deficient Stars through Common Envelope Evolution

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We present preliminary results from Smooth Particle Hydrodynamics (SPH) simulations of common envelope evolution. We qualitatively compare the interaction between a 0.9M red giant with two different companion masses: a 0.05M brown dwarf and a 0.25M white dwarf companion.
4 pages, 3 figures, Proceedings of the "Hydrogen Deficient Stars" meeting, Tuebingen, Germany, 2007

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/141309

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0711.0322
 http://arxiv.org/abs/0711.0322

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arXiv