Computer Science
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3084..238b&link_type=abstract
In its The Interstellar Medium in External Galaxies: Summaries of Contributed Papers p 238-240 (SEE N91-14100 05-90)
Computer Science
1
Galaxies, Hydrogen, Interstellar Matter, Luminosity, Molecular Gases, Orion Nebula, Star Formation, Comparison, Fluorescence, Line Spectra, Photodissociation, Solar Radiation
Scientific paper
The total shocked and fluorescent molecular hydrogen 1-0 S(1) line
luminosities from Orion have been measured to be about 2.5 solar
luminosity and about 2.0 solar luminosity, respectively. The
implications for using Orion to study the interstellar medium in
galaxies is discussed.
Burton Michael
Puxley Phil J.
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