Star formation seen with high resolution spectroscopy.

Details Star formation seen with high resolution spectroscopy. Star formation seen with high resolution spectroscopy.

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jmost.217..363w&link_type=abstract

J. Mol. Struct., Vol. 217, special issue, Part A, p. 363 - 369

Physics

1

Molecular Clouds: Spectroscopy, Molecular Clouds: Organic Molecules

Scientific paper

More than 90 anorganic and organic molecules have been detected by high resolution spectroscopy in interstellar molecular clouds or in the envelopes of stars. The detected wavelengths of the lines - predominantly located in the millimeter- and submillimeter wavelength region - unequivocally identify the molecules and give precise knowledge of the physical and chemical conditions of molecular clouds from which the radiation emanates. The line intensities and line profiles contain information about the densities, temperatures and dynamics prevailing in molecular clouds.

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