An analytical approximation of post-shock conditions in type II supernova shells

Details An analytical approximation of post-shock conditions in type II supernova shells An analytical approximation of post-shock conditions in type II supernova shells

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...386..711n&link_type=abstract

Astronomy and Astrophysics, v.386, p.711-720 (2002)

Astronomy and Astrophysics

Astrophysics

2

Stars: Supernovae: General, Shock Waves, Nuclear Reactions, Nucleosynthesis, Abundances

Scientific paper

We describe simple analytical formulae constructed to approximate the temporal behavior of the temperature, density, and radius of various presupernova shells immediately after the arrival of the supernova shock wave. The formulae are derived from detailed hydrodynamical simulation of the supernova envelope expulsion. When used within traditional nuclear kinetic codes, the formulae are expected to be a useful tool for adjusting the resulting nuclear yields to current supernova models.

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