Volume 612, April 2018
|Number of page(s)||6|
|Section||Atomic, molecular, and nuclear data|
|Published online||03 May 2018|
Excitation and charge transfer in low-energy hydrogen atom collisions with neutral iron★
Theoretical Astrophysics, Department of Physics and Astronomy, Uppsala University,
Accepted: 26 December 2017
Data for inelastic processes due to hydrogen atom collisions with iron are needed for accurate modelling of the iron spectrum in late-type stars. Excitation and charge transfer in low-energy Fe+H collisions is studied theoretically using a previously presented method based on an asymptotic two-electron linear combination of atomic orbitals model of ionic-covalent interactions in the neutral atom-hydrogen-atom system, together with the multi-channel Landau–Zener model. An extensive calculation including 166 covalent states and 25 ionic states is presented and rate coefficients are calculated for temperatures in the range 1000–20 000 K. The largest rates are found for charge transfer processes to and from two clusters of states around 6.3 and 6.6 eV excitation, corresponding in both cases to active 4d and 5p electrons undergoing transfer. Excitation and de-excitation processes among these two sets of states are also significant.
Key words: atomic data / atomic processes / line: formation / Sun: abundances / stars: abundances
Full Tables and rate coefficient data are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (22.214.171.124) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/612/A90
© ESO 2018
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