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Ro-vibrational excitation of CS by He
2006
Astronomy and Astrophysics
Context. Over the next few years, ALMA and Herschel missions will perform high spatial and spectral resolution studies at infrared and sub-millimeter wavelengths. Modeling of the spectra will require accurate radiative and collisional rates for species of astrophysical interest. Aims. The present paper focuses on the calculation of ro-vibrational excitation rate coefficients of CS by He, useful for studies of high-temperature interstellar environments. Methods. A new accurate three dimensional
doi:10.1051/0004-6361:20066422
fatcat:stjwqrgsw5hj5cvrg7p26bqlsu