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Continuum radio emission from the Magellanic Clouds

Published online by Cambridge University Press:  14 August 2015

D. S. Mathewson  and
J. R. Healey
D. S. Mathewson
Affiliation:
CSIRO Radiophysics Laboratory, Sydney
J. R. Healey
Affiliation:
CSIRO Radiophysics Laboratory, Sydney

Extract

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Before discussing the results of the radio observations of the Magellanic Clouds in detail, it is worth while to briefly review some of our current ideas about radio emission from “normal” galaxies which would be the classification given to the Clouds by radio astronomers. A “normal” galaxy has no striking visual peculiarity and has a much lower ratio of radio to light flux than the “radio” galaxy.

Type
Section II: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 245 - 255
Copyright
Copyright © Australian Academy of Science 1964 

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