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Supernova Remnants in Nearby Spiral Galaxies

Published online by Cambridge University Press:  12 April 2016

Knox S. Long
Knox S. Long*
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

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Large samples of supernova remnants are needed in order to study the global distribution of supernovae in galaxies, for determining how the environment in which a SN explodes affects the appearance of a SNR, for studying abundances and abundance gradients in galaxies, for estimating SN rates, and in order to determine the energetics of SNRs and their expansion. Here we describe techniques which are currently being used to expand SNR samples in nearby spirals.

Type
Supernova Remnants
Information
International Astronomical Union Colloquium , Volume 145: Supernovae and Supernova Remnants , 1996 , pp. 349 - 356
Copyright
Copyright © Cambridge University Press 1996

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