A multi-molecular study of the dense high-latitude cloud MCLD 126.6+24.5

Details A multi-molecular study of the dense high-latitude cloud MCLD 126.6+24.5 A multi-molecular study of the dense high-latitude cloud MCLD 126.6+24.5

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...268..255b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 268, no. 1, p. 255-264.

Astronomy and Astrophysics

Astrophysics

8

Abundance, Interstellar Matter, Line Spectra, Molecular Clouds, Chemical Composition, Electron Transitions, Molecular Excitation, Radio Spectra

Scientific paper

The translucent high-latitude cloud MCLD 126.6+24.5 has been studied on linear scales of a about 0.1 pc in (C-12)O, (C-13)O, and H2CO and 0.02 pc in NH3. The cloud shows structure on both scales. The integrated line intensities of (C-12)O, (C-13)O, and H2CO are linearly correlated with the IRAS 100 micron intensity. These correlations are used to derive the abundance for these molecules. The abundance of CO and H2CO is likely to be high for the cloud, and the NH3 abundance is normal compared to these values for dark clouds.

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