Cloud modeling with millimetre transitions: Implications for submillimetre observations

Details Cloud modeling with millimetre transitions: Implications for submillimetre observations Cloud modeling with millimetre transitions: Implications for submillimetre observations

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.189..109v&link_type=abstract

In ESA The Sci. Importance of Submillimetre Observations p 109-113 (SEE N83-22034 11-88)

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Cloud Cover, Galactic Rotation, Line Spectra, Molecular Clouds, Submillimeter Waves

Scientific paper

The implications of spectral line observations in the frequency range 200-350 GHz for techniques which infer physical properties of galactic molecular clouds are reviewed. Millimeter observations at high frequencies have made it possible to study several transitions of abundant molecules which improved the determination of temperatures and densities. The submillimeter region is an advantageous and powerful extension.

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