Nine successive rotational lines in the ground vibrational state of CS and C 34 S 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 10 8 up to 500 GHz and 5 parts in 10 8 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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Gottlieb et al. (2003) studied this question.
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