Sub-Chandrasekhar models for Type Ia supernovae and astrophysical transients
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
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|Source:||Proceedings of Science|
|01_Fink_Sub-Chandrasekhar_models_for_2013.pdf||1.58 MB||Adobe PDF||Request a copy|
|02_Fink_Sub-Chandrasekhar_models_for_2013.pdf||87.88 kB||Adobe PDF||Request a copy|
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