加载中…
{\bf R}-matrix calculations combined with the adiabatic nuclei approximation are used to compute electron-impact rotiational excitation rates for three closed-shell diatomic cations, HeH, CH, ArH. Comparisons with previous studies show that an improved treatment of threshold effects leads to significant changes in the low temperature rates, furthermore the new calculations suggest that excitation of CH is dominated by transitions as is expected for cations with a large dipole moment. A model for ArH excitation in the Crab Nebula is presented which gives results consistent with the observations for electron densities in the range $2-3\times 10^3^{-3}$.

生成讲解博客的中文版本

生成AI智能校验的中文版本