Type Ia Supernova models arising from different distributions of igniting points

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dc.contributor	Universitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear
dc.contributor	Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
dc.contributor.author	García Senz, Domingo
dc.contributor.author	Bravo Guil, Eduardo
dc.date	2005-02
dc.identifier.citation	Garcia, D.; Bravo, E. Type Ia Supernova models arising from different distributions of igniting points. "Astronomy and astrophysics", Febrer 2005, vol. 430, núm. 2, p. 585-602.
dc.identifier.citation	0004-6361
dc.identifier.citation	10.1051/0004-6361:20041628
dc.identifier.uri	http://hdl.handle.net/2117/18820
dc.language.iso	eng
dc.relation	http://www.edpsciences.org
dc.rights	info:eu-repo/semantics/openAccess
dc.subject	Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject	Supernovae
dc.subject	Supernoves
dc.title	Type Ia Supernova models arising from different distributions of igniting points
dc.type	info:eu-repo/semantics/publishedVersion
dc.type	info:eu-repo/semantics/article
dc.description.abstract	In this paper we address the theory of type Ia supernovae from the moment of carbon runaway up to several hours after the explosion. We have concentrated on the boiling-pot model: a deflagration characterized by the (nearly-) simultaneous ignition of a number of bubbles that pervade the core of the white dwarf.
dc.description.abstract	Peer Reviewed