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Stark widths of Lu II spectral lines

  • Regular Article - Plasma Physics
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Abstract

Stark widths for 19 lines in the spectrum of singly charged lutetium ion have been calculated using modified semiempirical method for an electron density of \(10^{17}\hbox { cm}^{-3}\) and temperatures from 5 000 K up to 80 000 K. The obtained results have been used for the investigation of the influence of Stark broadening on Lu II spectral lines in stellar atmospheres and for the investigations of Stark width regularities. In the case of Lu II lines considered in this work, Stark broadening is important for white dwarfs but can be neglected in A-type star atmospheres.

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Data Availibility Statement

This manuscript has associated data in a data repository. [Authors’ comment: All data are in the article and can be obtained from authors. Later, they will be implemented in the STARK-B database https://starkb.obspm.fr/].

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Acknowledgements

This work has been supported with a STSM visit grant for M.S.D. within the framework of COST Action CA 18104 “Revealing the Milky Way with GAIA”.

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Authors and Affiliations

  1. Astronomical Observatory, Volgina 7, 11060, Belgrade, Serbia

    Milan S. Dimitrijević

  2. CNRS, LERMA, Observatoire de Paris, Sorbonne Université, Université PSL, 92190, Meudon, France

    Milan S. Dimitrijević

  3. Department of Applied Physics, Technical University-Sofia, 1000, Sofia, Bulgaria

    Magdalena Christova

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  1. Milan S. Dimitrijević
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  2. Magdalena Christova
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Both authors were involved in the preparation of the manuscript. Both authors have read and approved the final manuscript.

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Correspondence to Milan S. Dimitrijević.

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Dimitrijević, M.S., Christova, M. Stark widths of Lu II spectral lines. Eur. Phys. J. D 75, 172 (2021). https://doi.org/10.1140/epjd/s10053-021-00179-4

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