Molecular gas in 30 Doradus.

Details Molecular gas in 30 Doradus. Molecular gas in 30 Doradus.

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998msngr..93...38r&link_type=abstract

The Messenger, vol. 93, p. 38-42

Physics

2

Star-Forming Regions: Carbon Monoxide, Star-Forming Regions: Magellanic Clouds

Scientific paper

The 30 Doradus region contains luminous clusters of massive young stars emitting intense UV radiation and powerful stellar winds which have created loops and shells of ionised gas, and shows evidence for a highly efficient formation mechanism unmatched in Galactic molecular clouds. The authors summarise here the results of an ongoing investigation of the characteristics of the highly excited molecular gas and cold molecular gas toward the centre of the 30 Doradus region, made through observations of H2 and CO(2→1) line emission, respectively.

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