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Sub-Chandrasekhar models for Type Ia supernovae and astrophysical transients

Fink, M; Ropke, F. K.; Sim, Stuart A; Kromer, M; Seitenzahl, I. R.; Ruiter, A. J.; Hillebrandt, Wolfgang


Sub-Chandrasekhar models aim to explain Type Ia supernovae from the explosion of white dwarf stars with masses below the Chandrasekhar limit. An advantage of this scenario is the wide range of possible progenitor masses, which may lead to a wide range of

CollectionsANU Research Publications
Date published: 2013
Type: Conference paper
Source: Proceedings of Science


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