Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-12-12
Astron.Astrophys.450:655-666,2006
Astronomy and Astrophysics
Astrophysics
12 pages, 11 figures, submitted to A&A
Scientific paper
10.1051/0004-6361:20054052
In the framework of the Chandrasekhar-mass deflagration model for Type Ia supernovae (SNe Ia), a persisting free parameter is the initial morphology of the flame front, which is linked to the ignition process in the progenitor white dwarf. Previous analytical models indicate that the thermal runaway is driven by temperature perturbations (''bubbles'') that develop in the white dwarf's convective core. In order to probe the conditions at ignition (diameters, temperatures and evolutionary timescales), we have performed hydrodynamical 2D simulations of buoyant bubbles in white dwarf interiors. Our results show that fragmentation occurring during the bubble rise affects the outcome of the bubble evolution. Possible implications for the ignition process of SNe Ia are discussed.
Brüggen Marcus
Hillebrandt Wolfgang
Iapichino Luigi
Niemeyer Jens C.
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