Stark Broadening of Zn III Spectral Lines

被引：1
|
作者：
Dimitrijevic, Milan S. [1 ,2 ]
Christova, Magdalena D. [3 ]
机构：
[1] Astron Observ, Volgina 7, Belgrade 11060, Serbia
[2] Univ PSL, Sorbonne Univ, Observ Paris, LERMA,CNRS, F-92190 Meudon, France
[3] Tech Univ Sofia, Dept Appl Phys, Sofia 1000, Bulgaria
来源：
UNIVERSE | 2022年 / 8卷 / 08期
关键词：
Stark broadening; Zn III; line profiles; atomic data; atomic processes; line formation; stellar atmospheres; PLASMA; WIDTHS; ATMOSPHERES; DIAGNOSTICS; ALPHA; ZINC; HOT;
D O I：
10.3390/universe8080430
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Stark widths for spectral lines within 24 multiplets of Zn III singlets and triplets have been calculated using modified semiempirical method for an electron density of 10(17) cm(-3) and temperatures from 5000 K up to 100,000 K. The obtained results have been used for the investigation of the influence of Stark broadening on Zn III spectral lines in stellar atmospheres and for the considerations of Stark width similarites within supermultiplets and transition arrays.
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页数：11
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