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Stark Width Data for Tb II, Tb III and Tb IV Spectral Lines

Author

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  • Milan S. Dimitrijević

    (Astronomical Observatory, 11060 Belgrade, Serbia
    Sorbonne Université, Observatoire de Paris, Université PSL, CNRS, LERMA, F-92190 Meudon, France)

Abstract

A dataset of Stark widths for Tb II, Tb III and Tb IV is presented. To data obtained before, the results of new calculations for 62 Tb III lines from 5d to 6p j (6,j) o , a transition array, have been added. Calculations have been performed by using the simplified modified semiempirical method for temperatures from 5000 to 80,000 K for an electron density of 10 17 cm − 3 . The results were also used to discuss the regularities within multiplets and a supermultiplet.

Suggested Citation

  • Milan S. Dimitrijević, 2021. "Stark Width Data for Tb II, Tb III and Tb IV Spectral Lines," Data, MDPI, vol. 6(3), pages 1-12, March.
  • Handle: RePEc:gam:jdataj:v:6:y:2021:i:3:p:28-:d:512510
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    References listed on IDEAS

    as
    1. Milan S. Dimitrijević, 2020. "Forty Years of the Applications of Stark Broadening Data Determined with the Modified Semiempirical Method," Data, MDPI, vol. 5(3), pages 1-17, August.
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