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arXiv · 0711.0322

The Formation of Hydrogen Deficient Stars through Common Envelope Evolution

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.

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Steven Diehl, Chris Fryer, Falk Herwig. 2007-11-02. The Formation of Hydrogen Deficient Stars through Common Envelope Evolution. https://arxiv.org/abs/0711.0322

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