Hostname: page-component-5cf477f64f-tx7qf Total loading time: 0 Render date: 2025-04-06T21:17:19.276Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Bodenheimer, P and Woosley, S.E. Astrophys.J. (1983) 269, 281 CrossRefGoogle Scholar
Clark, D.H and Caswell, J.L. Mon.Not.Roy.Ast.Soc. (1976) 174, 267 CrossRefGoogle Scholar
Mills, B.Y. Proc.Astron.Soc.Aust. (1981) 4, 156 CrossRefGoogle Scholar
Tenorio-Tagle, G, Bodenheimer, P. and Yorke, H.W. Astron. and Astrophys. (1985) 145, 70 Google Scholar
Whiteoak, J.B. and Gardner, F.F. Astrophys. J. (1968) 154, 807 CrossRefGoogle Scholar