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Influence of Stark broadening of ionized chromium spectral lines in Ap-star atmospheres
The European Physical Journal D ( IF 1.5 ) Pub Date : 2021-08-26 , DOI: 10.1140/epjd/s10053-021-00244-y Abeer Almodlej 1 , Nabil Ben Nessib 1, 2 , Milan S. Dimitrijević 3
中文翻译:
Ap-star大气中电离铬谱线Stark展宽的影响
更新日期:2021-08-26
The European Physical Journal D ( IF 1.5 ) Pub Date : 2021-08-26 , DOI: 10.1140/epjd/s10053-021-00244-y Abeer Almodlej 1 , Nabil Ben Nessib 1, 2 , Milan S. Dimitrijević 3
Affiliation
Abstract
The influence of Stark broadening in ionized chromium spectral lines observed in stellar atmospheres of Ap stars is considered. We have calculated the fitting coefficients of these lines and used them to compare Stark broadening and thermal Doppler widths for the conditions in the atmosphere of the Ap-star HD 188041. We also studied the influence of the Stark broadening on a synthetic profile of a line in the spectrum of this star.
Graphic abstract
中文翻译:
Ap-star大气中电离铬谱线Stark展宽的影响
摘要
考虑了在 Ap 星的恒星大气中观察到的电离铬谱线中斯塔克展宽的影响。我们已经计算了这些线的拟合系数,并使用它们来比较 Ap-star HD 188041 大气条件下的斯塔克展宽和热多普勒宽度。我们还研究了斯塔克展宽对合成线剖面的影响在这颗恒星的光谱中。