Physical conditions in molecular clouds derived from sub-mm and far-IR spectroscopic observations

Details Physical conditions in molecular clouds derived from sub-mm and far-IR spectroscopic observations Physical conditions in molecular clouds derived from sub-mm and far-IR spectroscopic observations

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8925082s&link_type=abstract

Presented at the International Symposium on Submillimeter and Millimeter Astronomy, Kona, HI, 3-6 Oct. 1988

Astronomy and Astrophysics

Astronomy

Carbon, Infrared Astronomy, Molecular Clouds, Molecular Spectroscopy, Radio Sources (Astronomy), Absorption Spectra, Brightness Distribution, Clumps, Galactic Nuclei, Nebulae

Scientific paper

Knowledge about the warm, dense component discovered in all reasonably high luminosity sources in the galaxy is summarized and observations in the fine structure lines of neutral and ionized atomic carbon are discussed. The best explanation for the observed extended emission in these lines is its origin in photodissociation regions on clump surfaces in a clumpy UV penetrated cloud.

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