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The Magellanic Cloud Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

Michael A. Dopita
Michael A. Dopita*
Affiliation:
Mt. Stromlo & Siding Spring Observatories, Research School of Physical Sciences, Australian National University, Canberra

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It was some twenty years ago, at the previous IAU symposium devoted to the Magellanic Clouds, that Mathewson and Healey (1964) announced the discovery of the first supernova remnant (SNR) in the LMC. The method used was to identify a non-thermal radio source with a filamentary optical emission object and this confirmed N49 in the catalogue of Henize (1956) as an SNR and suggested N63 and N132 D as likely candidates.

Information

Type
Supernova Remnants, Radio Continuum, X-ray Sources
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984, pp. 271 - 281
Copyright
Copyright © Reidel 1984 

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