Rotational excitation of CS and SiO by collisions with Helium

Astronomy and Astrophysics – Astrophysics

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Scientific paper

The modelisation of line intensities as a result of molecular excitation calculations requires accurate values of the radiative transfer coefficients and collisional excitation rates, corresponding to collisional processes with the most abundant neutral species, He and H_2. We present new sets of rotational excitation rate coefficients for the SiO-He and CS-He colliding systems, calculated among the 31 (CS) and 26 (SiO) first rotational states for temperatures ranging from 5 to 300 K. These data were obtained from reliable quantum chemical calculations, using 2D SiO-He and CS-He potential energy surfaces and close-coupling calculations of the collisional excitation cross sections. Features of the obtained excitation cross sections, such as their associated propensity rules, were further analyzed.

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