ACCURATE COLLISIONAL CROSS-SECTIONS: IMPORTANT NON-LTE INPUT DATA

被引:3
作者
Mashonkina, L. [1 ]
机构
[1] Russian Acad Sci, Inst Astron, Moscow 119017, Russia
来源
NON-LTE LINE FORMATION FOR TRACE ELEMENTS IN STELLAR ATMOSPHERES | 2010年 / 43卷
关键词
METAL-POOR STARS; COOL DWARF STARS; RADIATIVE TRANSITION RATES; ATOM-ATOM COLLISIONS; LINE FORMATION; RATE COEFFICIENTS; HYDROGEN-ATOMS; HEAVY-ELEMENTS; ABUNDANCES; EXCITATION;
D O I
10.1051/eas/1043006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Non-LTE modelling for a particular atom requires accurate collisional excitation and ionization cross-sections for the entire system of transitions in the atom. This review concerns with inelastic collisions with electrons and neutral hydrogen atoms. For the selected atoms, H I and Ca II, comparisons are made between electron impact excitation rates from ab initio calculations and various theoretical approximations. The effect of the use of modern data on non-LTE modelling is shown. For most transitions and most atoms, hydrogen collisional rates are calculated using a semi-empirical modification of the classical Thomson formula for ionization by electrons. Approaches used to estimate empirically the efficiency of hydrogenic collisions in the statistical equilibrium of atoms are reviewed.
引用
收藏
页码:79 / 90
页数:12
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