Zooming into the remarkable southern hot core G327.3-0.6 and its environs

Details Zooming into the remarkable southern hot core G327.3-0.6 and its environs Zooming into the remarkable southern hot core G327.3-0.6 and its environs

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..388w&link_type=abstract

ATNF proposal C1588, Semester: April, 2006

Computer Science

Galactic, Atca

Scientific paper

There is no generally accepted evolutionary scheme for high mass star formation yet. A simple approach to address this problem is to cover several of the known stages during the formation of massive stars in the same cloud and then investigate their properites. Recent APEX observations of the massive hot core G327.3-0.6 found a massive cold N2H+ clump in the environs of the hot core. Here we propose 3mm ATCA observations of both, the hot and the cold core, to spatially resolve the cores. The combination of APEX and ATCA has a great potential in obtaining a complete view of the region, which large scale morphology and large spectral coverage of many lines from different molecules with a large range of excitation observed with APEX, and a detailed view of the small scale morphology and kinematics with the ATCA interferometer. This will lead to a comprehensive view in this template source of two important stages during the formation of massive stars.

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