High-excitation rotational molecular lines from dense interstellar clouds

Details High-excitation rotational molecular lines from dense interstellar clouds High-excitation rotational molecular lines from dense interstellar clouds

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.189...31s&link_type=abstract

In ESA The Sci. Importance of Submillimetre Observations p 31-32 (SEE N83-22034 11-88)

Mathematics

Brightness Temperature, Line Spectra, Molecular Clouds, Molecular Rotation, Thermalization (Energy Absorption), Boltzmann Distribution, Carbon Monoxide, Dipole Moments, Excitation, Mathematical Models, Velocity Distribution

Scientific paper

A simple mode is presented for evaluating the intensities of carbon monoxide rotational lines from dense molecular clouds. The calculations are performed for optically thin lines and a thermal distribution in the level population, in agreement with data on the observed high transitions. The calculated brightness temperatures seem to allow observational detection.

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