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Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2010

Inelastic Na+H collision data for non-LTE applications in stellar atmospheres

P.S. Barklem
  • Fonction : Auteur
A. K. Belyaev
  • Fonction : Auteur
A. D. Dickinson
  • Fonction : Auteur
Florent X. Gadéa

Résumé

Rate coefficients for inelastic Na+H collisions are calculated for all transitions between the ten levels up to and including the ionic state (ion-pair production), namely Na(3s,3p,4s,3d,4p,5s,4d,4f,5p)+H(1s) and Na++H-. The calculations are based on recent full quantum scattering cross-section calculations. The data are needed for non-LTE applications in cool astrophysical environments, especially cool stellar atmospheres, and are presented for a temperature range of 500-8000 K. From consideration of the sensitivity of the cross-sections to input quantum chemical data and the results of different methods for the scattering calculations, a measure of the possible uncertainties in the rate coefficients is estimated.

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Dates et versions

hal-00841331 , version 1 (04-07-2013)

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Citer

P.S. Barklem, A. K. Belyaev, A. D. Dickinson, Florent X. Gadéa. Inelastic Na+H collision data for non-LTE applications in stellar atmospheres. Astronomy and Astrophysics - A&A, 2010, 519 (A20), pp.20. ⟨10.1051/0004-6361/201015152⟩. ⟨hal-00841331⟩
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