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.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
