The influence of the ortho:para-H2 ratio on molecular collisions in interstellar clouds.

Details The influence of the ortho:para-H2 ratio on molecular collisions in interstellar clouds. The influence of the ortho:para-H2 ratio on molecular collisions in interstellar clouds.

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991coamp..26...35f&link_type=abstract

Comments At. Mol. Phys., Vol. 26, No. 1, p. 35 - 45

Other

Interstellar Clouds: Molecular Processes, Interstellar Clouds: Atomic Processes

Scientific paper

Hydrogen is the most abundant molecule in interstellar clouds and plays a determining role in reactive and non-reactive scattering processes. The two forms of hydrogen - ortho- and para-H2 - can behave differently in collisions with other atomic and molecular species. The ortho:para ratio generally differs from its value in thermal equilibrium. Techniques for deducing this ratio are discussed which depend on theoretical and experimental determinations of collision cross-sections.

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