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The Dominant Interactions Between SNR and the ISM

Published online by Cambridge University Press:  12 April 2016

Robert Braun
Robert Braun*
Affiliation:
National Radio Astronomy Observatory*, P.O. Box O, Socorro, New Mexico 87801, USA

Abstract

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The interactions of supernovae ejecta with the surrounding medium which have a dominant influence on the resulting SNR dynamics and brightness are considered for both young and evolved objects. The important roles of clumpy ejecta in determining the brightness of young SNR and of shock impingement on a pre-existing shell in influencing both the brightness and subsequent dynamics of evolved SNR are stressed.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 227 - 230
Copyright
Copyright © Cambridge University Press 1988

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