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Paper: The Formation of Hydrogen Deficient Stars through Common Envelope Evolution
Volume: 391, Hydrogen-Deficient Stars
Page: 221
Authors: Diehl, S.; Fryer, C.; Herwig, F.
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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