Structure and physical conditions of the dense gas in the Monoceros R2 molecular cloud

Details Structure and physical conditions of the dense gas in the Monoceros R2 molecular cloud Structure and physical conditions of the dense gas in the Monoceros R2 molecular cloud

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...233..527m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 233, no. 2, July 1990, p. 527-534. Research supported by CAICYT.

Astronomy and Astrophysics

Astrophysics

14

Interstellar Gas, Line Spectra, Molecular Clouds, Star Formation, Ultraviolet Spectra, Ammonia, Carbon Monoxide, Carbon 13, Gas Density, H Ii Regions, Infrared Stars, Photodissociation

Scientific paper

Observations of (C-13)O, S, and NH3 in the Mon R2 molecular cloud are
presented. The existence of a dense 3-pc 4000-solar mass region is
revealed. The high-resolution observations of the (1,1) and (2,2) lines
of NH3 show the presence of 1-65-solar mass clumps. A minimum in the NH3
emission is observed toward the compact H II region.

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