Thermal Evolution of AM CVn Binary Donors

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dc.creatorDeloye, Christopher J.
dc.creatorTaam, Ronald E.
dc.creatorWinisdoerffer, Christophe
dc.creatorChabrier, Gilles
dc.date2006-10-20
dc.date.accessioned2026-07-07T07:27:03Z
dc.date.available2026-07-07T07:27:03Z
dc.descriptionWe discuss results of our study on AM CVn binaries formed with donors that never ignited He before contact. For the first time, we treat the donor's in these systems in the context of a full stellar structure evolution theory and find that the binary's evolution can described in terms of 3 phases: contact, adiabatic donor expansion, and late-time donor cooling. Details of the first and third phase are new results from this study and we focus on generally characterizing these two phases. Finally, we present our predictions for the donor's light in these systems.
dc.descriptionTo appear in Proc 15th European White Dwarf Workshop, held in Leicester Aug 7-11th 2006, and to be published by ASP
dc.identifierhttps://arxiv.org/abs/astro-ph/0610609
dc.identifierhttp://arxiv.org/abs/astro-ph/0610609
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117245
dc.subjectAstrophysics
dc.titleThermal Evolution of AM CVn Binary Donors
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