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Radiative processes affecting the abundance of interstellar OHPhotodissociation 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.
Document ID
19760057942
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/154544
Authors
Smith, w. H. (Princeton Univ. Observatory NJ, United States)
Zweibel, E. G. (Princeton University New Observatory, Princeton, N.J., United States)
Date Acquired
August 8, 2013
Publication Date
August 1, 1976
Publication Information
Publication: Astrophysical Journal
Volume: 207
Subject Category
Astrophysics
Accession Number
76A40908
Funding Number(s)
CONTRACT_GRANT: NSF MPS-71-03108A03
CONTRACT_GRANT: NGL-31-001-007
Distribution Limits
Public
Copyright
Other

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