The rates of rotational transitions for HCO+, the most abundant ion in interstellar space, induced by collision with helium are obtained for temperatures ranging from 10 to 80 K. The calculations are based on a new potential energy surface for the He-HCO+ interaction and on a scattering matrix whose accuracy was checked by pressure broadening and shift measurements. The rates decrease for increasing values of j and Δj, with a temperature trend depending on the energy involved in the transitions: if it is small, the rates are almost constant, while an increase with T is found for other cases. Comparison with previous and less accurate results shows an agreement within 50 per cent. Comparison between state-to-state and pressure broadening cross-sections allows us to discuss importance and influence of elastic and inelastic collisions. © 2009 The Authors. Journal compilation © 2009 RAS.
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Buffa, G., Dore, L., & Meuwly, M. (2009). State-to-state rotational transition rates of the HCO+ ion by collisions with helium. Monthly Notices of the Royal Astronomical Society, 397(4), 1909–1914. https://doi.org/10.1111/j.1365-2966.2009.14890.x