Rate coefficients for the rotational excitation of CO by ortho- and para-H2

Details Rate coefficients for the rotational excitation of CO by ortho- and para-H2 Rate coefficients for the rotational excitation of CO by ortho- and para-H2

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214..271f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 15, 1985, p. 271-277.

Astronomy and Astrophysics

Astronomy

166

Carbon Monoxide, Hydrogen Clouds, Interstellar Chemistry, Interstellar Gas, Molecular Excitation, Molecular Rotation, Coefficients, Microwave Spectra, Molecular Clouds, Ortho Hydrogen, Para Hydrogen, Quantum Mechanics, Rates (Per Time), Submillimeter Waves

Scientific paper

Rate coefficients for the rotational excitation of 12C16O by ortho- and para-H2 are given for the low-temperature regime of interstellar molecular clouds. The rate coefficients derive from quantum mechanical coupled channels calculations of the relevant cross-sections and are intended for the analysis of the intensities of CO microwave and submillimetre lines.

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