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Extragalactic supernova remnantsBecause the supernova remnants (SNRs) in other galaxies are at well-defined distances and because in many cases the reddening within extragalactic samples is more uniform than is the case for the Galactic SNR sample, extragalactic SNRs are fundamental to improving the understanding of SNR evolution. Here methods for identifying SNRs are reviewed and the current status of observational research is explored. The data do not unambiguously support the simple Sedov picture of SNR expansion, although it may be that the data can be reconciled with this picture if sufficient variation in initial conditions is allowed.
Document ID
19850067166
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Long, K. S.
(Johns Hopkins University Baltimore, MD, United States)
Date Acquired
August 12, 2013
Publication Date
April 1, 1985
Publication Information
Publication: Space Science Reviews
Volume: 40
ISSN: 0038-6308
Subject Category
Astrophysics
Accession Number
85A49317
Funding Number(s)
CONTRACT_GRANT: NAS5-27000
Distribution Limits
Public
Copyright
Other

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