An Expanded Study of Molecular Regions in the Magellanic Bridge

Details An Expanded Study of Molecular Regions in the Magellanic Bridge An Expanded Study of Molecular Regions in the Magellanic Bridge

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop..789m&link_type=abstract

ATNF proposal M136, Semester: April, 2007

Physics

Mag Clouds, Mopra

Scientific paper

We will continue our search for the ultra small-scale and weak molecular clouds in the tenuous and tidal filament, the Magellanic Bridge. We will use the brightest molecular tracer, the CO(1-0) transition in an effort to locate, and parameterise the se molecular regions. The Bridge is one of the most poorly metallic, yet one of the closest objects to our Galaxy, and is able to provide unprecidented resolution for future studies of starformation in unenriched environments. As a first step in this work, we aim to continue to locate the CO emission regions to high resolution Using the Mopra telescope. This work is ongoing, although we will adopt a scanning technique in an effort to improve observing efficiency.

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