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arxiv: 1510.05101 · v1 · pith:USEXSQ6Bnew · submitted 2015-10-17 · 🌌 astro-ph.GA

Electron-impact excitation of diatomic hydride cations I: HeH^+, CH^+, ArH^+

classification 🌌 astro-ph.GA
keywords excitationcationscalculationsdiatomicelectron-impactratesadiabaticapproximation
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{\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 $\Delta J =1$ 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 $2-3\times 10^3$~cm$^{-3}$.

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