A Three-Dimensional Deflagration Model for Type Ia Supernovae Compared with Observations
A simulation of the thermonuclear explosion of a Chandrasekhar-mass C+O white dwarf, the most popular scenario of a Type Ia supernova (SN Ia), is presented. The underlying modeling is pursued in a self-consistent way, treating the combustion wave as a turbulent deflagration using well tested methods...
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Veröffentlicht in: | The Astrophysical journal 2007-10, Vol.668 (2), p.1132-1139 |
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Format: | Artikel |
Sprache: | eng |
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