Completion of high resolution mapping of CO within the SMC

Details Completion of high resolution mapping of CO within the SMC Completion of high resolution mapping of CO within the SMC

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop..810m&link_type=abstract

ATNF proposal M186, Semester: April, 2007

Computer Science

Mag Clouds, Mopra

Scientific paper

We intend to extend our successful observataions of the south-western SMC into the remaining CO-bright regions in the north and sout east of the metal-poor and tidally peturbed dwarf Small Magellanic Cloud. In doing so, we will complete mapping the significant and detectable CO emission regions in the SMC, at the highest resolutions currently possible. Many of the molecular clouds in the SMC can only be resolved using the Mopra telescope and we will finally be able to confidently correlate the properties of the molecular regions as a function of their location within the ihhomgenous SMC; as a comparison across the rest of the Magellanic System (against existing and underway measurements of CO regions in the LMC and Bridge) ; and also against molecular clouds in the Galaxy.

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