Stark Broadening of Zn III Spectral Lines

Stark widths for spectral lines within 24 multiplets of Zn III singlets and triplets have been calculated using modified semiempirical method for an electron density of 1017 cm−3 and temperatures from 5000 K up to 100,000 K. The obtained results have been used for the investigation of the influence...

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Veröffentlicht in:Universe (Basel) 2022-08, Vol.8 (8), p.430
Hauptverfasser: Dimitrijević, Milan S., Christova, Magdalena D.
Format: Artikel
Sprache:eng
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Zusammenfassung:Stark widths for spectral lines within 24 multiplets of Zn III singlets and triplets have been calculated using modified semiempirical method for an electron density of 1017 cm−3 and temperatures from 5000 K up to 100,000 K. The obtained results have been used for the investigation of the influence of Stark broadening on Zn III spectral lines in stellar atmospheres and for the considerations of Stark width similarites within supermultiplets and transition arrays.
ISSN:2218-1997
2218-1997
DOI:10.3390/universe8080430