Photodissociation rates of molecules by the interstellar radiation field

Details Photodissociation rates of molecules by the interstellar radiation field Photodissociation rates of molecules by the interstellar radiation field

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...282..172l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 282, July 1, 1984, p. 172-177.

Astronomy and Astrophysics

Astrophysics

57

Interstellar Chemistry, Interstellar Radiation, Molecular Clouds, Photodissociation, Abundance, Carbon Monoxide, Interstellar Matter, Methane, Molecular Interactions, Nitrogen Oxides, Radiation Distribution, Rates (Per Time), Sulfur Dioxides, Water

Scientific paper

The photodissociation rates of CO, NO, H2O, HCN, NO2, SO2, CS2, OCS, NH3, CH4, H2O2, and C2H2, dissociated by the interstellar ultraviolet background in the solar neighborhood are calculated for the 106 - 200 nm wavelength region. The processes for photodissociation of various interstellar molecules into fragments are discussed.

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