The infrared emission lines of H2

Details The infrared emission lines of H2 The infrared emission lines of H2

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.163..333z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 163, no. 2, Jan. 1990, p. 333-339. Research supported by the Institute of

Astronomy and Astrophysics

Astrophysics

Hydrogen, Infrared Spectra, Molecular Clouds, Molecular Spectra, Photodissociation, Emission Spectra, Fluorescence, Interstellar Matter, Ortho Para Conversion

Scientific paper

The photodissociation regions located between ionized regions and molecular clouds are studied by using a one-dimensional model where molecular H2 are formed on the dust grains and destructed by photodissociation. The escape probability method is used for the line transfer. The excitation of IR emission lines of H2 by UV fluorescence in M17, by shock heating in Orion KL and mainly by UV fluorescence in NGC 2023 are discussed.

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