Aims. Rate coefficients for inelastic Al + H and Al+ + H− collisions are calculated for all transitions between the seven low-lying levels up to and including the ionic state, namely Al(3p,4s,3d,4p,5s,nd)+H(1s) and Al+ + H−. The data are needed for non-LTE applications in stellar atmospheres and are presented for a temperature range of 1000–10 000 K.
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A. K. Belyaev (2013) studied this question.
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