A 3mm Line Survey Towards Sites of Massive Star Formation

Details A 3mm Line Survey Towards Sites of Massive Star Formation A 3mm Line Survey Towards Sites of Massive Star Formation

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..109w&link_type=abstract

ATNF proposal M168, Semester: April, 2006

Physics

Galactic, Mopra

Scientific paper

Previous spectral line surveys have revealed a wealth of new information on the chemistry of star formation. However, less than a dozen sources have been targeted, the bulk of the work being performed towards just two (Orion-KL and Sgr B2). With the recently upgraded Mopra telescope, we aim to survey 57 sources across the entire 3mm band, increasing the number of spectral line survey sources by a factor of five. The results will be used to identify chemical markers (clocks) of the various stages of massive star formation.

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