The thermal evolution of mass losing donors in AM CVn binary systems

Taam, R. E; Deloye, C. J; Sengupta, S

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4799

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DC Field	Value	Language
dc.contributor.author	Taam, R. E	-
dc.contributor.author	Deloye, C. J	-
dc.contributor.author	Sengupta, S	-
dc.date.accessioned	2009-09-08T14:27:23Z	-
dc.date.available	2009-09-08T14:27:23Z	-
dc.date.issued	2009-08	-
dc.identifier.citation	B. Soonthornthum, S. Komonjinda, K.S. Cheng, and K.C. Leung., eds., The Eighth Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conference Series, Vol. 404, Proceedings of the Conference held 5 - 9 May, 2008, at Merlin Beach Hotel, Phuket, Thailand., pp. 241 – 247	en
dc.identifier.isbn	978-1-58381-685-1	-
dc.identifier.uri	http://hdl.handle.net/2248/4799	-
dc.description	Restricted Access	-
dc.description.abstract	The thermal evolution of arbitrarily degenerate stellar models for the mass losing component in AM CVn binary systems formed through the white dwarf evolutionary channel is investigated for a range of initial orbital periods and initial system masses. Based on these models, the evolutionary phases and properties of AM CVn binary systems are described and the observational signature of their donors is discussed.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.ispartofseries	ASP Conference Series;Vol. 404	-
dc.relation.uri	http://aspbooks.org/custom/publications/paper/404-0241.html	en
dc.rights	© Astronomical Society of the Pacific	en
dc.subject	Thermal Evolution	en
dc.subject	Mass Losing Donors	en
dc.subject	AM CVn Binary Systems	en
dc.title	The thermal evolution of mass losing donors in AM CVn binary systems	en
dc.type	Article	en
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