The Formation of Hydrogen Deficient Stars through Common Envelope Evolution

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dc.creatorDiehl, Steven
dc.creatorFryer, Chris
dc.creatorHerwig, Falk
dc.date2007-11-02
dc.date.accessioned2026-07-07T08:40:12Z
dc.date.available2026-07-07T08:40:12Z
dc.descriptionWe 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.
dc.description4 pages, 3 figures, Proceedings of the "Hydrogen Deficient Stars" meeting, Tuebingen, Germany, 2007
dc.identifierhttps://arxiv.org/abs/0711.0322
dc.identifierhttp://arxiv.org/abs/0711.0322
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/141309
dc.subjectAstrophysics
dc.titleThe Formation of Hydrogen Deficient Stars through Common Envelope Evolution
dc.typetext

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