The infrared spectrum of CS

Details The infrared spectrum of CS The infrared spectrum of CS

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984cajph..62.1414w&link_type=abstract

Canadian Journal of Physics (ISSN 0008-4204), vol. 62, Dec. 1984, p. 1414-1419.

Physics

11

Astronomical Spectroscopy, Carbon Compounds, Infrared Spectra, Interstellar Matter, Sulfides, Power Spectra, Spectral Bands, Spectrum Analysis

Scientific paper

The (Delta-v)=2 IR emission bands of the X1Sigma(+) state of gaseous (C-12)(S-32) and (C-12)(S-34) are investigated experimentally using the Fourier-transform spectrometer at Kitt Peak National Solar Observatory. The results are presented in tables and characterized. Of the eight bands (containing up to 200 lines each) identified for (C-12)(S-32), the strongest head is that of 2-0 at 2585/cm, with the other heads toward smaller wavenumbers separated by about 26/cm. The interest of these transitions for astrophysical studies of the emissions of C-rich stars, molecular clouds, and comets is indicated.

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