Breit-Pauli energy levels, transition probabilities and lifetimes for 3d5 levels in FeIV of astrophysical interest

被引：10

作者：

Fischer, CF

Rubin, RH

机构：

[1] Vanderbilt Univ, Dept Comp Sci, Nashville, TN 37232 USA

[2] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA

[3] Orion Enterprises, Moffett Field, CA 94035 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2004年 / 355卷 / 02期

关键词：

atomic data; atomic processes;

D O I：

10.1111/j.1365-2966.2004.08332.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Energy levels, lifetimes and transition probabilities for transitions between computed levels of 3d(5) of Fe IV are reported. The E2 and M1 transition probabilities are compared with earlier theoretical results, often only the values published by Garstang in 1958. From the available astronomical observations of optical emission lines arising from the same level, a few direct tests are now possible and they show consistency with the theoretical calculations.

引用

收藏

页码：461 / 474

页数：14

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