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Radio Observations of Galactic SNRs

Published online by Cambridge University Press:  26 May 2016

D.A. Green
D.A. Green*
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE, U.K.

Abstract

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This paper reviews several aspects of the study of radio emission from Galactic Supernova Remnants (SNRs). The detection of radio emission from SNRs is the most important method for identification of SNRs, and the limitations imposed by selection effects on subsequent statistical studies are discussed. Also discussed are the spectral properties of SNRs, both their integrated spectra, and the evidence for spectral variations across the face of remnants.

Type
Part 5: Galactic Surveys and Extended Emission
Information
Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 276 - 283
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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