Radio Continuum Emission from Methanol Maser Sites

Details Radio Continuum Emission from Methanol Maser Sites Radio Continuum Emission from Methanol Maser Sites

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..456w&link_type=abstract

ATNF proposal C865, Semester: October, 2006

Computer Science

Galactic, Atca

Scientific paper

Class II methanol maser emission is closely related to IR-luminous sites of high mass star formation which are usually signposted by ultracompact HII regions. However, G305.2+0.2 contains two methanol maser sites, one with bright IR emission, but have no detected HII region. Our previous ATCA observations, which show the non-detections, also show an extended radio source offset from G305.2+0.2, which greatly affects our flux upper limit. We therefore propose to image the extended emission with compact ATCA configurations.

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