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Collective Effects in Shock Propagation Through a Clumpy Medium
Published online by Cambridge University Press: 12 April 2016
Abstract
A numerical simulation of shock propagation in a clumpy medium with a weak magnetic field is presented which illustrates a number of dynamical processes of potential importance for explaining spectral line width and radio polarization measurements in supernova remnants.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 223 - 226
- Copyright
- Copyright © Cambridge University Press 1988