Observational constraints on the origin of the elements - I. 3D NLTE formation of Mn lines in late-type stars

Maria Bergemann; Andrew J. Gallagher; Philipp Eitner; Manuel Bautista; Remo Collet; Svetlana A. Yakovleva; Anja Mayriedl; Bertrand Plez; Mats Carlsson; Jorrit Leenaarts; Andrey K. Belyaev; Camilla Hansen

doi:10.1051/0004-6361/201935811

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Volume 631 (November 2019)

A&A, 631 (2019) A80

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Fig. 3

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Neutralisation rate coefficients for Mn⁺(3d⁵4s ⁵S) + H⁻ collisions asa function of electronic energy in different excited states of Mn I. The dashed line represents the reduced rate coefficient given by the simplified model.

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