Precise Millimeter-Wave Laboratory Frequencies for CS and C34S

Details Precise Millimeter-Wave Laboratory Frequencies for CS and C34S Precise Millimeter-Wave Laboratory Frequencies for CS and C34S

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003apj...588..655g&link_type=abstract

The Astrophysical Journal, Volume 588, Issue 1, pp. 655-661.

Astronomy and Astrophysics

Astronomy

28

Ism: Molecules, Methods: Laboratory, Molecular Data, Molecular Processes, Radio Lines: Ism, Stars: Formation

Scientific paper

Nine successive rotational lines in the ground vibrational state of CS and C34S between 96 GHz (J=2-1) and 500 GHz (10-9) were measured in the laboratory to an accuracy of a few kHz. When our measurements are combined with the submillimeter-wave measurements of Ahrens & Winnewisser, the entire rotational spectrum of both isotopic species is predicted to an accuracy of about 1 part in 108 up to 500 GHz and 5 parts in 108 near 1000 GHz. These frequencies should be useful for quantitative studies of cloud core collapse and star formation in the millimeter- and submillimeter-wave bands.

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