Carbon monoxide in the Magellanic Clouds.

Computer Science

Scientific paper

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Magellanic Clouds: Carbon Monoxide

Scientific paper

Thanks to the good angular resolution of the SEST, much progress has been done on the properties of molecular gas in the Magellanic Clouds, and this is outlined in the paper. A substantial fraction of the Clouds has been mapped in the CO lines at a linear resolution of about 10 pc, sufficient to resolve the ordinary molecular clouds inside large gas complexes. Multi-line observations have allowed to explain why these clouds look different in CO than Galactic clouds.

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