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Instabilities and Mixing in Type II-P and II-b Supernovae
Published online by Cambridge University Press: 12 April 2016
Abstract
We calculate a nonlinear growth of the Rayleigh-Taylor instability in the exploding red supergiant stars with a two-dimensional hydrodynamical code, and examine how the extent of mixing depends on the progenitor's core mass and the envelope mass. The results are compared with the observations of type II-P supernovae and the recent type Il-b supernova 1993J.
- Type
- Type lb and Type II Supernovae
- Information
- International Astronomical Union Colloquium , Volume 145: Supernovae and Supernova Remnants , 1996 , pp. 129 - 135
- Copyright
- Copyright © Cambridge University Press 1996
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