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 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..368m&link_type=abstract

ATNF proposal M136, Semester: April, 2006

Physics

Mag Clouds, Mopra

Scientific paper

We propose to continue deep measurements of two CO-emission regions in the Magellanic Bridge, with the intent to expand the current number of resolved CO detections in the Magellanic Bridge from one, to three. In doing so, we will be in a position to provide accurate estimates of the spatial extent, position, and velocity widths of a range of different molecular regions in the Bridge, allowing the starforming potential and general ISM properties to be more fully understood overall in this unique and metal-poor structure.

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