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On the road to consistent Type Ia supernova explosion models

Published online by Cambridge University Press:  01 August 2006

Friedrich K. Röpke
Friedrich K. Röpke*
Affiliation:
Department of Astronomy and Astrophysics, University of California Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, USA Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany email: fritz@mpa-garching.mpg.de
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Abstract

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Keeping up with ever more detailed observations, Type Ia supernova (SN Ia) explosion models have seen a brisk development over the past years. The aim is to construct a self-consistent picture of the physical processes in order to gain the predictive power necessary to answer questions arising from the application of SNe Ia as cosmological distance indicators. We review recent developments in modeling these objects focusing on three-dimensional simulations.

Keywords

supernovae: generalhydrodynamicsmethods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 308 - 309
Copyright
Copyright © International Astronomical Union 2007

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