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Radio imaging of the supernova remnant N132D in the Large Magellanic Cloud

Published online by Cambridge University Press:  19 July 2016

John R. Dickel  and
D. K. Milne
John R. Dickel
Affiliation:
University of Illinois Astronomy Building, 1002 West Green Street, Urbana, IL 61801, U.S.A.
D. K. Milne
Affiliation:
Australia Telescope National Facility∗, P.O. Box 76, Epping, N.S.W. 2121, Australia

Abstract

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The first high resolution radio image of the supernova remnant N132D shows a complex shell structure.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 349 - 350
Copyright
Copyright © Kluwer 1991 

References

Mathewson, D.S., Ford, V.L., Dopita, M.A., Tuohy, I.R., Long, K.S. and Helfand, D.J. 1983, Astrophys. J. Suppl. 51, 345.Google Scholar