Can we estimate H$\mathsf{_{2}}$(<i>j</i>= 0) rate coefficients from He rate coefficients? Application to the SiS molecule

Abstract

Context.Over the next few years, the ALMA and Herschel missions will perform high spatial and spectral resolution studies at infrared and sub-millimeter wavelengths. Modeling of molecular emission requires excitation calculations using radiative, as well as collisional rates, with the most abundant species. In the interstellar medium, the dominant collision partner is H2, but little data is available for collisions with H2. If data for collisions with He are available, it has often been proposed to use the more available rate coefficients for collision with He, with the appropriate reduced mass correction, as a first estimate of rate coefficients with H2(). The validity of this approximation is not known.