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Supernova Remnants in the Large Magellanic Cloud: A Multiwavelength Study of Energetics and Environments

Published online by Cambridge University Press:  25 May 2016

Rosa Murphy Williams ,
You-Hua Chu ,
John R. Dickel  and
R. Chris Smith
Rosa Murphy Williams
Affiliation:
Astronomy Department, University of Illinois, Urbana, IL 61801, USA
You-Hua Chu
Affiliation:
Astronomy Department, University of Illinois, Urbana, IL 61801, USA
John R. Dickel
Affiliation:
Astronomy Department, University of Illinois, Urbana, IL 61801, USA
R. Chris Smith
Affiliation:
Cerro Tololo Inter-American Observatory, La Serena, Chile

Abstract

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We analyze optical, radio and X-ray data from supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) in order to make a systematic study of a full sample at a known distance. By this multiwavelength examination of SNRs from various progenitors and environments, we will build a comprehensive picture of the evolution of SNR structure and energetics.

Type
Part 2. Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 145 - 147
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Williams, R. M., et al. 1997, ApJ, 480, 618 CrossRefGoogle Scholar
Williams, R. M., et al. 1999, ApJ, 514, 798 Google Scholar