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Radio Emission from Supernova Remnants

Published online by Cambridge University Press:  07 February 2017

D. K. Milne
D. K. Milne*
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia

Abstract

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Observations of the radio emission from supernova remnants are reviewed with emphasis on the dissimilarity between the Crab Nebula and the other remnants. From this we conclude that there may be several non-thermal sources in the Galaxy with the same centrally filled structure as the Crab. These are, however, more evolved, and clearly there is no other source of the same age and type as the Crab Nebula.

Type
Session 4
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 248 - 262
Copyright
Copyright © Reidel 1971 

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