CO in 30 Doradus

Details CO in 30 Doradus CO in 30 Doradus

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...151..455m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 151, no. 2, Oct. 1985, p. 455, 456.

Astronomy and Astrophysics

Astrophysics

5

Carbon Monoxide, Magellanic Clouds, Molecular Clouds, H Ii Regions, Millimeter Waves, Stellar Evolution

Scientific paper

The authors have detected 12CO emission in the core of the giant H II region 30 Doradus in the LMC. The observed CO profiles are found to be much narrower than that of the ionized gas and it is unlikely that the molecular and atomic gas are well mixed within the nebula. The implications of these results to other giant extragalactic H II regions are discussed.

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