Morphology and kinematics of the molecular cloud associated with GM 24

Details Morphology and kinematics of the molecular cloud associated with GM 24 Morphology and kinematics of the molecular cloud associated with GM 24

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...234..447g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 234, no. 1-2, Aug. 1990, p. 447-453. Research supported by SEUI and Junta de A

Astronomy and Astrophysics

Astrophysics

3

Carbon Monoxide, H Ii Regions, Interstellar Gas, Molecular Clouds, Molecular Spectra, Morphology, Carbon 13, Oxygen 18, Spectral Line Width, Star Clusters

Scientific paper

The molecular cloud associated with GM 24 in the rotational transition lines of CO (J = 2-1), (C-13)O(J = 1-0), and C(O-18)(J= 1-0) is studied. It is found that there is significant enhancement of the C(O-18) and (C-13)O linewidths near the stellar activity center. It is found that the characteristics of the GM 24 molecular cloud, in terms of abundances of CO and its isotopic species, are similar to those of rho Ophiuchi and Taurus.

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