Stark broadening of CdI spectral lines

被引：26
作者：
Simic, Z
Dimitrijevic, MS
Milovanovic, N
Sahal-Bréchot, S
机构：
[1] Astron Observ, Belgrade 11160, Serbia Monteneg
[2] Observ Paris, F-92195 Meudon, France
来源：
ASTRONOMY & ASTROPHYSICS | 2005年 / 441卷 / 01期
关键词：
line : profiles; atomic data; atomic processes; lines formation; stars : atmospheres;
D O I：
10.1051/0004-6361:20052701
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Stark broadening parameters, widths, and shifts for 33 Cd I singlets and 37 triplets were calculated using the semi-classical perturbation method. The results were compared with available experimental and theoretical data. Also, regularity in the spectral series 5s(2) S-1-np P-1 degrees was investigated. The influence of Stark broadening was analyzed in A-type stellar atmospheres.
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收藏
页码：391 / 393
页数：3
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