The Formation of Hydrogen Deficient Stars through Common Envelope Evolution

Details The Formation of Hydrogen Deficient Stars through Common Envelope Evolution The Formation of Hydrogen Deficient Stars through Common Envelope Evolution

2007-11-02

arxiv.org/abs/0711.0322v1

Astronomy and Astrophysics

Astrophysics

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

Scientific paper

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.

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