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oai:recercat.cat:2117/188202026-01-18T07:02:20Zcom_2072_1033col_2072_452950

Type Ia Supernova models arising from different distributions of igniting points García Senz, Domingo Bravo Guil, Eduardo Universitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica Àrees temàtiques de la UPC::Física::Astronomia i astrofísica Supernovae Supernoves 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. Peer Reviewed Postprint (published version) 2005-02 Article 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. 0004-6361 https://hdl.handle.net/2117/18820 10.1051/0004-6361:20041628 eng http://www.edpsciences.org Open Access 18 p. application/pdf