Observations of ammonia in galactic H II regions

Details Observations of ammonia in galactic H II regions Observations of ammonia in galactic H II regions

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.141..339v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 141, no. 2, Feb. 1988, p. 339-346. Research supported by the Fundacao de A

Physics

Optics

2

Ammonia, H Ii Regions, Milky Way Galaxy, Molecular Clouds, Acousto-Optics, Physical Properties, Space Density

Scientific paper

This paper presents the first results for the (J,K) = (1,1) and (2,2)
ammonia transitions observed in the direction of some southern galactic
H II regions, selected among the strongest H2CO emitters. Some physical
parameters derived for each individual source, including several new
sources of ammonia lines, are presented.

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