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Determining the main-sequence mass of Type II supernova progenitors

Monthly Notices of the Royal Astronomical Society, no. 2 (2010): 827-840

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hydrodynamicsradiative transferstars: atmospheresstars: supernovae: general

Abstract

We present radiation–hydrodynamic simulations of core-collapse supernova (SN) explosions, artificially generated by driving a piston at the base of the envelope of a rotating or non-rotating red-supergiant progenitor star. We search for trends in ejecta kinematics in the resulting Type II-Plateau (II-P) SN, exploring dependencies with exp...More

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Luc Dessart

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Eli Livne

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Roni Waldman

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