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The Energetics of Type II Supernovae

  • Amos Yahil
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 109)

Abstract

The energetics of type II supernovae is considered within the gravitational implosion-explosion picture. The total (internal plus gravitational) energies of different parts of the star are calculated, when they are in, or close to, hydrostatic equilibrium. This enables an estimate of the energy transferred to other parts of the star, and ultimately to the supernova ejectum.

Keywords

Inner Core Composition Profile Outer Core Hydrostatic Equilibrium Nuclear Matter Density 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company 1984

Authors and Affiliations

  • Amos Yahil
    • 1
  1. 1.State University of New YorkStony BrookUSA

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