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Radio Properties of Magellanic Cloud SNRs

Published online by Cambridge University Press:  25 May 2016

John R. Dickel
John R. Dickel*
Affiliation:
Astronomy Department, University of Illinois, Urbana, IL 61801, USA

Abstract

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Supernova remnants in the Magellanic Clouds may have somewhat lower surface brightnesses at radio wavelengths than their counterparts in the Milky Way but otherwise they appear to be very similar. Balmer dominated SNRs have a lower radio luminosity than other shell remnants.

Type
Part 2. Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 139 - 140
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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