Theoretical values for the [O III] 5007/4959 line-intensity ratio and homologous cases

被引:482
作者
Storey, PJ
Zeippen, CJ
机构
[1] UCL, Dept Phys & Astron, London WC1E 6BT, England
[2] CNRS, UMR 8631, F-92195 Meudon, France
[3] Univ Paris 07, F-92195 Meudon, France
[4] Observ Paris, DAEC, F-92195 Meudon, France
关键词
atomic data; line : formation; techniques : spectroscopic; HII regions; planetary nebulae : general;
D O I
10.1046/j.1365-8711.2000.03184.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The magnetic-dipole probabilities for the (1)D(2)-(3)P(2) and (1)D(2)-(3)P(1) transitions in carbon-like and oxygen-like ions are calculated up to atomic number Z = 12, including relativistic corrections to the magnetic dipole operator. The ratio of the probabilities for these two transitions is found to change by up to 5 per cent compared with previous theoretical work, none of which included these relativistic corrections, with the effect being largest for the near neutral ions. The transition probability ratio for the [O III] 5007 and 4959 Angstrom lines is found to be 3.01, implying an intensity ratio of 2.98, in significantly better agreement with the observed ratio than the earlier theoretical work.
引用
收藏
页码:813 / 816
页数:4
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