A JCMT HARP survey of molecular outflows associated with 6.7 GHz methanol masers

Details A JCMT HARP survey of molecular outflows associated with 6.7 GHz methanol masers A JCMT HARP survey of molecular outflows associated with 6.7 GHz methanol masers

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011yera.confe..11d&link_type=abstract

The 41st Young European Radio Astronomers Conference, held at University of Manchester/Jodrell Bank Observatory, 18-20 July 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

The 6.7 GHz methanol maser is a valuable tracer of early massive star formation and is a promising candidate with which to unravel the early stages in the formation of a high mass star. Despite this promise, the precise evolutionary phase traced by the maser is not yet clear. I will describe the preliminary results of a JCMT HARP survey for outflows associated with methanol masers, which is aimed at determining the number, frequency and dynamical lifetime of outflows associated with the masers. I will also discuss the application of new 3D methods of outflow identification to the HARP Galactic Plane Survey.

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