Recombination coefficients for CII lines

被引:112
作者
Davey, AR
Storey, PJ
Kisielius, R
机构
[1] Montana State Univ, Dept Phys, Bozeman, MT 59717 USA
[2] UCL, Dept Phys & Astron, London WC1E 6BT, England
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 2000年 / 142卷 / 01期
关键词
atomic data; line : formation; HII regions; planetary nebulae : general;
D O I
10.1051/aas:2000139
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Effective recombination coefficients are given for CII transitions between doublet states. The calculations are carried out in the temperature range 500 - 20 000 K and for an electron density of 10(4) cm(-3) The effects of electron collisions on the excited states are included. The necessary bound-bound and bound-free radiative data are obtained from a new R-matrix calculation in which photoionization resonances are fully delineated, thereby accurately incorporating the effects of both radiative and dielectronic recombination. The R-matrix calculation includes all bound states with principal quantum number n less than or equal to 15 and total orbital angular momentum L less than or equal to 4. The effect of moving the resonance features to their experimentally determined positions is also investigated and found to be important at low temperatures.
引用
收藏
页码:85 / 94
页数:10
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