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Electron-impact excitation of diatomic hydride cations II: OH$^+$ and SH$^+$

Published 21 Feb 2018 in astro-ph.SR and astro-ph.GA | (1802.07566v1)

Abstract: R-matrix calculations combined with the adiabatic-nuclei-rotation and Coulomb-Born approximations are used to compute electron-impact rotational rate coefficients for two open-shell diatomic cations of astrophysical interest: the hydoxyl and sulphanyl ions, OH$+$ and SH$+$. Hyperfine resolved rate coefficients are deduced using the infinite-order-sudden approximation. The propensity rule $\Delta F=\Delta j=\Delta N=\pm 1$ is observed, as is expected for cations with a large dipole moment. A model for OH$+$ excitation in the Orion Bar photon-dominated region (PDR) is presented which nicely reproduces Herschel observations for an electron fraction $x_e=10{-4}$ and an OH$+$ column density of $3\times 10{13}$~cm${-2}$. Electron impact electronic excitation cross sections and rate coefficients for the ions are also presented.

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