Computer Science
Scientific paper
Apr 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976conm....1..123s&link_type=abstract
In its Contrib. of the Observatory of N. Mex. State Univ., Vol. 1, No. 4 p 123-133 (SEE N76-29085 19-89)
Computer Science
1
Emission Spectra, Hydrogen, Infrared Spectra, Transition Temperature, Chemical Composition, Interstellar Matter, Transition Flow
Scientific paper
The emissivities of the infrared rotational transitions of H2 are
calculated for temperatures from 10 K to 6000 K. The calculations are
made for several ratios, R, of Para (J=0) to Ortho (J=1)H2. The
possibility of detecting these transitions in interstellar molecular
clouds is discussed.
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