The fine spatial structure of methanol masers

Details The fine spatial structure of methanol masers The fine spatial structure of methanol masers

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43..785s&link_type=abstract

Astronomy Reports, Volume 43, Issue 12, December 1999, pp.785-796

Astronomy and Astrophysics

Astronomy

3

Scientific paper

The results of mapping the structure of five methanol masers (M8E, W33Met, G14.33-0.64, L379IRS3, and GGD27) in the 7_0-6_1 A+ transition at 7 mm with an angular resolution of 0.1" are presented. Some masers form chains of bright, unresolved maser spots, extended along curved lines or arcs. The length of these arcs is from 20 to 1000 AU. The brightness temperatures of the strongest masers exceed 3.6 x 10^8 K. The distributions of the maser spots are consistent with the hypothesis that they originate at interfaces between molecular outflows and ambient molecular clouds.

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