Interstellar carbon monosulfide

Details Interstellar carbon monosulfide Interstellar carbon monosulfide

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196..709l&link_type=abstract

Astrophysical Journal, vol. 196, Mar. 15, 1975, pt. 1, p. 709-717.

Astronomy and Astrophysics

Astronomy

50

Carbon Compounds, Interstellar Matter, Sulfides, Galactic Structure, H Ii Regions, Radiative Transfer, Radio Astronomy

Scientific paper

We have measured intensities of the J = 3-2, 2-1, and 1-0 transitions of carbon monosulfide in five molecular clouds associated with galactic H II regions. The two higher-lying lines were mapped in each source, and the lowest line, J = 1-0, was observed at the map centers. The observed intensity ratios are shown to be dominated by effects of instrumental resolution. The observations are corrected for these effects and discussed in terms of recently published calculations for radiative transfer in collapsing clouds.

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