Molecular Gas in the Magellanic Clouds

Details Molecular Gas in the Magellanic Clouds Molecular Gas in the Magellanic Clouds

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.6202i&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #62.02; Bulletin of the American Astronomical Society, Vol. 30, p.906

Astronomy and Astrophysics

Astronomy

Scientific paper

We discuss the properties of dense interstellar clouds in the low-metallicity environment of the Magellanic Clouds, based on CO, C(+) and infrared observations. In this environment, radiation dominates the physical processes, leading to a significant variety in the appearance and properties of the molecular cloud complexes. The importance of high-freqency observations possible from Antarctica will be put in the context of using Magellanic Cloud conditions as a template for observations of star-forming galaxies at high redshift.

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