Stark Widths of Yb III and Lu IV Spectral Lines
AbstractRare Earth Elements are important for stellar atmosphere analysis but the corresponding Stark broadening data are scarce. For Yb III and Lu IV theoretical as well as experimental data on Stark broadening parameters of spectral lines are absent in the literature. Using the modified semiempirical method of Dimitrijević and Konjević, we determined Stark widths for four Yb III and four Lu IV transitions, belonging to the erbium isoelectronic sequence. The obtained results are also used to discuss similarities between homologous transitions in the erbium isoelectronic sequence. We note as well that calculated widths will be implemented in the STARK-B database which is also a part of the Virtual Atomic and Molecular Data Center. View Full-Text
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Dimitrijević, M.S. Stark Widths of Yb III and Lu IV Spectral Lines. Atoms 2019, 7, 10.
Dimitrijević MS. Stark Widths of Yb III and Lu IV Spectral Lines. Atoms. 2019; 7(1):10.Chicago/Turabian Style
Dimitrijević, Milan S. 2019. "Stark Widths of Yb III and Lu IV Spectral Lines." Atoms 7, no. 1: 10.
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