Inelastic e+Mg collision data and its impact on modelling stellar and supernova spectra
Results of calculations for inelastic e+Mg effective collision strengths for the lowest 25 physical states of Mg i (up to 3s6p1P), and thus 300 transitions, from the convergent close-coupling (CCC) and the B-spline R-matrix (BSR) methods are presented. At temperatures of interest, 5000 K, the results of the two calculations differ on average by
Barklem, P. S. et al.
Fecha de publicación:
9
2017