Infrared Diagnostics of the Formation of H 2 on Interstellar Dust

Details Infrared Diagnostics of the Formation of H 2 on Interstellar Dust Infrared Diagnostics of the Formation of H 2 on Interstellar Dust

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...449..178l&link_type=abstract

Astrophysical Journal v.449, p.178

Astronomy and Astrophysics

Astronomy

25

Infrared: Ism: Lines And Bands, Ism: Clouds, Ism: Dust, Extinction Infrared, Ism: Molecules

Scientific paper

The infrared spectrum arising from the formation of molecular hydrogen in molecular clouds is calculated for three different possible mechanisms. The contribution to the spectrum arising from the excitation of molecular hydrogen by cosmic ray secondary electrons is included. Specific emission lines that may serve as diagnostics of the formation mechanism are identified.

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