• Milan S. Dimitrijević 1. Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia; 2. Sorbonne Université, Observatoire de Paris, Université PSL, CNRS, LERMA, F-92190, Meudon, France
Keywords: Stark broadening, Spectral lines, Line profiles, Tb III


Stark full widths at half maximum (FWHM) for 26 6s-6p transitions in Tb III spectrum have been calculated for electron density of 1017 cm-3 within a temperature range of 5 000 K to 80 000 K, by using the simplified modified semiempirical (SMSE) method. The results obtained are used for the consideration of Strak width regularities within the investigated transition array.


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