Cool gas in southern galaxies.

Details Cool gas in southern galaxies. Cool gas in southern galaxies.

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998msngr..91...45h&link_type=abstract

The Messenger, vol. 91, p. 45-48

Astronomy and Astrophysics

Astrophysics

Magellanic Clouds: Star-Forming Regions, Magellanic Clouds: Molecules, Starburst Galaxies: Molecules, Starburst Galaxies: Star-Forming Regions

Scientific paper

The Magellanic Clouds provide an extremely interesting environment to study astrophysical processes. With respect to the molecular interstellar medium, there are three outstanding properties which motivate ongoing research: (1) Metallicities are smaller than in the Milky Way, (2) UV radiation fields are stronger than in the solar neighbourhood, and (3) a large number of targets is found at a well-known (relatively small) distance. The first two properties have far-reaching consequences for the astrophysical and astrochemical state of the interstellar medium.

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