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The Evolution of Supernova Remnants as Radio Sources

Published online by Cambridge University Press:  04 August 2017

R. Cowsik  and
S. Sarkar
R. Cowsik
Affiliation:
Tata Institute of Fundamental Research, Homi Bhabha Road, Bombay 400005, India
S. Sarkar*
Affiliation:
Tata Institute of Fundamental Research, Homi Bhabha Road, Bombay 400005, India
*
Now at Department of Astrophysics, University of Oxford, South Parks Road, Oxford OX1 3RQ, England

Abstract

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The acceleration of relativistic electrons by hydromagnetic turbulence in shell-type supernova remnants (SNRs) is examined within the framework of previous studies of their structural evolution through interaction with the interstellar medium. The predicted evolution of the synchrotron radio emission by the electrons is in agreement with a wide variety of observations.

Type
I. Young Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 187 - 192
Copyright
Copyright © Reidel 1983 

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