Rotational excitation of OH by para-H2:rate coefficients calculated in an intermediate coupling representation

Details Rotational excitation of OH by para-H2:rate coefficients calculated in an intermediate coupling representation Rotational excitation of OH by para-H2:rate coefficients calculated in an intermediate coupling representation

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.226..505d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 226, May 15, 1987, p. 505-512.

Astronomy and Astrophysics

Astrophysics

44

Ground State, Hydroxyl Radicals, Molecular Collisions, Molecular Excitation, Molecular Rotation, Para Hydrogen, Astrophysics, Interstellar Masers, Potential Energy, Quantum Mechanics, Reaction Kinetics

Scientific paper

Rate coefficients are presented for the rotational excitation of OH by para-H2 in its rotational ground state. The authors believe that these results will be useful for astrophysical studies of the far-infrared rotational transitions of OH, as well as the OH masers. An outstanding discrepancy in the potential energy expansion for the OH-H2 system is also discussed.

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