Atomic data from the IRON Project .27. Electron impact excitation collision strengths and rate coefficients for FeIV

被引:63
作者
Zhang, HL
Pradhan, AK
机构
[1] Department of Astronomy, Ohio State University, Columbus
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1997年 / 126卷 / 02期
关键词
atomic processes; planetary nebulae; general; H II regions;
D O I
10.1051/aas:1997388
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Collision strengths and maxwellian-averaged rate coefficients have been calculated for 8771 non-vanishing transitions among 140 fine structure levels, dominated by the configurations 3d(5), 3d(4)4s, and 3d(4)4p in Fe IV. Collision strengths are calculated using the R-matrix method with a 49 term close-coupling target expansion for electron energies up to 15 rydbergs. Rate coefficients are tabulated for a wide range of temperatures in which Fe IV is abundant in plasma sources. A brief discussion of the calculations and sample results are given. The present rates for Fe IV are expected to find applications in spectral diagnostics of a variety of astrophysical sources.
引用
收藏
页码:373 / 378
页数:6
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