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).
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References
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MATHEWSON, D., HEALEY, J. & WESTERLUND, B. A Supernova Remnant in the Large Magellanic Cloud. Nature 199, 681 (1963). https://doi.org/10.1038/199681a0
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DOI: https://doi.org/10.1038/199681a0
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