Rate constants for rotational transitions of CO scattered by para-hydrogen

Details Rate constants for rotational transitions of CO scattered by para-hydrogen Rate constants for rotational transitions of CO scattered by para-hydrogen

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...299..939s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 299, Dec. 15, 1985, p. 939-946.

Statistics

Computation

93

Carbon Monoxide, Computational Astrophysics, Hydrogen Clouds, Molecular Clouds, Molecular Rotation, Para Hydrogen, Approximation, Molecular Interactions, Temperature Distribution

Scientific paper

Rate constants for the collisional excitation of CO by para-hydrogen are calculated in the temperature range 5 ≤ T ≤ 2000K using the coupled states approximaton and a recently determined new potential surface. The results differ appreciably at high temperatures and large Δj transitions from those recently used in the interpretation of shock wave models in molecular clouds.

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