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Low Mach Number Modeling of Type Ia Supernovae. IV. White Dwarf Convection

ASTROPHYSICAL JOURNAL, no. 1 (2009): 196-210

Cited by: 73|Views4

Abstract

We present the first three-dimensional, full-star simulations of convection in a white dwarf preceding a Type Ia supernova, specifically the last few hours before ignition. For these long-time calculations, we use our low Mach number hydrodynamics code, MAESTRO, which we have further developed to treat spherical stars centered in a three-...More

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