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Barrel-Shaped Supernova Remnants

Published online by Cambridge University Press:  12 April 2016

M.J. Kesteven  and
J.L. Caswell
M.J. Kesteven
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76 Epping, NSW, Australia, 2121
J.L. Caswell
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76 Epping, NSW, Australia, 2121

Abstract

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We argue that the majority of radio supernova remnants have a three-dimensional distribution of emissivity which is barrel shaped, with little emission from the end-caps. We examine some mechanisms which could produce this distribution.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 359 - 361
Copyright
Copyright © Cambridge University Press 1988

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