NASA NTRS · 19760057942
Radiative processes affecting the abundance of interstellar OH
Abstract
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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Smith, w. H., Zweibel, E. G.. 1976-08-01. Radiative processes affecting the abundance of interstellar OH. https://ntrs.nasa.gov/citations/19760057942
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