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A search for non-thermal emission in the HII regions of the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

S. W. Amy
S. W. Amy*
Affiliation:
School of Physics, University of Sydney, Sydney, NSW 2006, Australia

Abstract

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The 843 MHz radio survey of the Magellanic Clouds with the Molonglo Observatory Synthesis Telescope (MOST) has provided continuum images with a resolution of about 45 arcsec for many HII regions. By comparing these radio data with H-alpha data regions of non-thermal emission may be found within HII regions.

Type
Star Formation and Clustering
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 195
Copyright
Copyright © Kluwer 1991