Modeling of iron K lines:: Radiative and auger decay data for FeII-FeIX

被引:116
作者
Palmeri, P
Mendoza, C
Kallman, TR
Bautista, MA
Meléndez, M
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Inst Venezolano Invest Cient, Ctr Fis, Caracas 1020A, Venezuela
关键词
atomic data; atomic processes; techniques : spectroscopic;
D O I
10.1051/0004-6361:20031262
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A detailed analysis of the radiative and Auger de-excitation channels of K- shell vacancy states in Fe II - Fe IX has been carried out. Level energies, wavelengths, A-values, Auger rates and fluorescence yields have been calculated for the lowest fine-structure levels populated by photoionization of the ground state of the parent ion. Different branching ratios, namely Kalpha(2) /Kalpha(1), Kbeta/ Kalpha, KLM /KLL, KMM /KLL, and the total K-shell fluorescence yields, omega(K), obtained in the present work have been compared with other theoretical data and solid-state measurements, finding good general agreement with the latter. The Kalpha(2) /Kalpha(1) ratio is found to be sensitive to the excitation mechanism. From these comparisons it has been possible to estimate an accuracy of similar to 10% for the present transition probabilities.
引用
收藏
页码:359 / 364
页数:6
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