Nov 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008eas....32..283i&link_type=abstract
EAS Publications Series, Volume 32, 2008, pp.283-310
Physics
1
Scientific paper
Type Ia supernovae are thought to be the outcome of the thermonuclear explosion of a carbon oxygen white dwarf in a close binary system. In this review we discuss the observational background, the possible progenitors, the mechanisms leading to the instability and the development of the explosion itself as well as the remaining uncertainties.
Bravo Eduardo
Hirschmann A.
Isern Jordi
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