K-shell photoionization and electron impact excitation of Fe XVII-Fe XXIII

被引:34
作者
Bautista, MA
Mendoza, C
Kallman, TR
Palmeri, P
机构
[1] Inst Venezolano Invest Cient, Ctr Fis, Caracas 1020A, Venezuela
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
关键词
atomic data; atomic processes; line : formation;
D O I
10.1051/0004-6361:20034198
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Photoabsorption cross sections across the K edge of Fe XVII-Fe XXIII and electron impact K-shell excitation effective collision strengths in Fe XVIII-Fe XXIII have been computed with the Breit-Pauli R-matrix method. The target models are represented with all the fine-structure levels within the n=2 complex, built up from single-electron orbital bases obtained in a Thomas-Fermi-Dirac statistical model potential. The effects of radiation and spectator Auger dampings are taken into account by means of an optical potential. In photoabsorption, these effects cause the resonances converging to the K thresholds to display symmetric profiles of constant width that smear the edge, with important implications in spectral analysis. In collisional excitation, they attenuate resonances making their contributions to the effective collision strength practically negligible.
引用
收藏
页码:1171 / 1178
页数:8
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