High Resolution Imaging of Bipolar Molecular Outflows in the G333 Cloud

Details High Resolution Imaging of Bipolar Molecular Outflows in the G333 Cloud High Resolution Imaging of Bipolar Molecular Outflows in the G333 Cloud

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..362b&link_type=abstract

ATNF proposal C1583, Semester: April, 2006

Other

Galactic, Atca

Scientific paper

We have an ongoing programme using Mopra molecular line data to investigate the role played by turbulence in triggering and regulating star formation in the G333 giant molecular cloud. To make a comprehensive assessment of this role, we also require information on the feedback effect of YSOs within the cloud. We have selected 6 bright molecular regions in the Mopra data, 4 of which are associated with bipolar molecular outflows and all of which that are associated with UCHII regions, to image with ATCA in molecular species specifically chosen for their outflow diagnostic properties. The data will provide a higher resolution study of the known Mopra outflows and the opportunity to detect suspected outflows in the other 2 sources that are likely compromised by the large Mopra beam size. In this way we will be able to investigate the return of energy and momentum to the cloud and elucidate whether the turbulence generated in this way could be sufficient to influence a future generation of star formation. This is part of a multi-wavelength, international campaign to study star formation in the G333 cloud and provide benchmarking observational contraints on the role played by turbulence in this process.

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