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Type Ia Supernovae

Published online by Cambridge University Press:  06 November 2008

C. Charbonnel ,
J.-P. Zahn ,
J. Isern ,
E. Bravo  and
A. Hirschmann
J. Isern
Affiliation:
Institut de Ciències de l'Espai (CSIC – IEEC) & Institut d'Estudis Espacials de Catalunya, Torre C-5 parells 2n, Campus UAB, 08193 Bellaterra, Spain
E. Bravo
Affiliation:
Departament de Física i Enginyeria Nuclear (UPC) & Institut d'Estudis Espacials de Catalunya, Diagonal 647, 08028 Barcelona, Spain
A. Hirschmann
Affiliation:
Departament de Física i Enginyeria Nuclear (UPC) & Institut d'Estudis Espacials de Catalunya, Diagonal 647, 08028 Barcelona, Spain
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Abstract

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.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 32: Stellar Nucleosynthesis: 50 years after B2FH , 2008 , pp. 283 - 310
Copyright
© EAS, EDP Sciences, 2008

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