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The Formation of Hydrogen Deficient Stars through Common Envelope Evolution

Astrophysics 2007-11-05 v1
Authors: Steven Diehl , Chris Fryer , Falk Herwig
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Abstract

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.

Keywords

dwarf galaxies stellar and substellar companions white dwarfs

Cite

@article{arxiv.0711.0322,
  title  = {The Formation of Hydrogen Deficient Stars through Common Envelope Evolution},
  author = {Steven Diehl and Chris Fryer and Falk Herwig},
  journal= {arXiv preprint arXiv:0711.0322},
  year   = {2007}
}

Comments

4 pages, 3 figures, Proceedings of the "Hydrogen Deficient Stars" meeting, Tuebingen, Germany, 2007

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