Radiative processes affecting the abundance of interstellar OH

Details Radiative processes affecting the abundance of interstellar OH Radiative processes affecting the abundance of interstellar OH

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...207..758s&link_type=abstract

Astrophysical Journal, vol. 207, Aug. 1, 1976, pt. 1, p. 758-762.

Astronomy and Astrophysics

Astrophysics

15

Abundance, Hydroxyl Radicals, Interstellar Matter, Photodissociation, Radiative Recombination, H I Regions, Ionic Reactions, Molecular Interactions, Radiation Shielding

Scientific paper

Photodissociation of OH dominates its destruction for a significant
range of density and shielding in H I regions. Although inverse
predissociation may provide an observable flux of ultraviolet
recombination photons, it can provide only a small fraction of the total
observed OH in most H I regions.

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