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The Galactic distribution of SNRs

Published online by Cambridge University Press:  29 January 2014

D. A. Green
D. A. Green*
Affiliation:
Cavendish Laboratory, 19 J. J. Thomson Ave., Cambridge, CB3 0HE, U.K. email: [email protected]
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Abstract

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It is not straightforward to determine the distribution of supernova remnants (SNRs) in the Galaxy. The two main difficulties are that there are observational selection effects that mean that catalogues of SNRs are incomplete, and distances are not available for most remnants. Here I discuss the selection effects that apply to the latest catalogue of Galactic SNRs. I then compare the observed distribution of ‘bright’ SNRs in Galactic longitude with that expected from models in order to constrain the Galactic distribution of SNRs.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 188 - 196
Copyright
Copyright © International Astronomical Union 2014 

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