Electron-impact rotational and hyperfine excitation of HCN, HNC, DCN and DNC

Abstract

Rotational excitation of isotopologues of HCN and HNC by thermal electron-impact is studied using the molecular {\bf R}-matrix method combined with the adiabatic-nuclei-rotation (ANR) approximation. Rate coefficients are obtained for electron temperatures in the range 5$-$6000 K and for transitions among all levels up to J=8. Hyperfine rates are also derived using the infinite-order-sudden (IOS) scaling method. It is shown that the dominant rotational transitions are dipole allowed, that is those for which $\Delta J=1$. The hyperfine propensity rule $\Delta J=\Delta F$ is found to be stronger than in the case of He$-$HCN collisions. For dipole allowed transitions, electron-impact rates are shown to exceed those for excitation of HCN by He atoms by 6 orders of magnitude. As a result, the present rates should be included in any detailed population model of isotopologues of HCN and HNC in sources where the electron fraction is larger than 10${}^{-6}$, for example in interstellar shocks and comets.

12 pages, 4 figures, accepted in MNRAS (2007 september 3)

References in corpus (4)

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• The Excitation of N${}_2$H${}^{+}$ in Interstellar Molecular Clouds. I - Models
• Detection of HNC and tentative detection of CN at z=3.9
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