Oscillator strengths for transitions in O III

被引：29

作者：

Aggarwal, KM

Hibbert, A

Keenan, FP

机构：

[1] UNIV DELHI,DEPT PHYS & ASTROPHYS,DELHI 110007,INDIA

[2] QUEENS UNIV BELFAST,DEPT APPL MATH & THEORET PHYS,BELFAST BT7 1NN,ANTRIM,NORTH IRELAND

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 1997年 / 108卷 / 01期

关键词：

atomic data;

D O I：

10.1086/312949

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Energy levels and oscillator strengths have been calculated for the fine-structure transitions among the levels of the (1s(2)) 2s(2)2p(2), 2s2p(3), 2p(4), 2s(2)2p3s, 2s(2)2p3p, and 2s(2)2p3d configurations of O III using the CIV3 program. The extensive configuration interaction and relativistic effects have been included while generating the wave functions. The results are compared with other recent theoretical estimates, and their accuracy is assessed.

引用

收藏

页码：393 / 401

页数：9

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