Abstract
THE proximity of the Large Magellanic Cloud offers an unparalleled opportunity for the detailed comparison of an external galaxy at optical and radio wave-lengths. Recently the 210-ft. steerable reflector at the Australian National Radio Astronomy Observatory has been used to survey the Large Cloud at a number of wave-lengths between 11 cm and 220 cm. The results of this work have been presented at the recent International Astronomical Union/International Scientific Radio Union Symposium No. 20 (ref. 1).
Similar content being viewed by others
Article PDF
References
Mathewson, D. S., and Healey, J. R., I.A.U./U.R.S.I. Symp. No. 20 (1963).
Dickel, H. R., Aller, L. H., and Faulkner, D. J., I.A.U./U.R.S.I. Symp. No. 20 (1963).
Doherty, L., Henize, K. G., and Aller, L. H., Astrophys. J., Supp. No. 22, 2, 345 (1956).
Henize, K. G., Astrophys. J., Supp. No. 22, 2, 315 (1956).
Mills, B. Y., Slee, O. B., and Hill, E. B., Austral. J. Phys., 14, 497 (1961).
Minkowski, R., and Aller, L. H., Astrophys. J., 119, 232 (1954).
Shklovsky, I. S., U.S.S.R. Astro. J., 4, 243 (1960).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
MATHEWSON, D., HEALEY, J. & WESTERLUND, B. A Supernova Remnant in the Large Magellanic Cloud. Nature 199, 681 (1963). https://doi.org/10.1038/199681a0
Issue Date:
DOI: https://doi.org/10.1038/199681a0
This article is cited by
-
Radio emission from supernova remnants
The Astronomy and Astrophysics Review (2015)
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.