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Studies of SNRS in the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

A. J. Turtle
A. J. Turtle*
Affiliation:
School of Physics, University of Sydney, Sydney, NSW 2006, Australia

Abstract

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In the Magellanic Clouds about 60 confirmed supernova remnants (SNRs) or candidates are known. They have been detected by a combination of X-ray, optical and radio observations. Various statistical aspects of these SNRs will be considered including the implied supernova rate, the spatial distribution, the implications of the radio luminosity/diameter distribution for SNR evolution, and the relation to the extended non-thermal emission.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 313
Copyright
Copyright © Kluwer 1991