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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
Abstract
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
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- Copyright © Kluwer 1991