Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/955
Title: On the Stark broadening of Te I spectral lines for CP star plasma analysis
Authors: Dimitrijević, M. S.
Simić, Z.
Kovačević, Anđelka 
Dačić, M.
Sahal-Bréchot, S.
Affiliations: Astronomy 
Keywords: Atomic data;Atomic processes;Line: formation;Line: profiles;Stars: atmospheres;Stars: chemically peculiar
Issue Date: 1-Apr-2008
Related Publication(s): CP#AP workshop 2007
Journal: Contributions of the Astronomical Observatory Skalnate Pleso
Abstract: 
By using the semiclassical perturbation method, Stark widths and shifts have been calculated for the Te I 6s 5So - 7p 5p (5125.2 Å) multiplet, of interest for CP star plasma studies. Results were applied to the investigation of the influence of Stark broadening on CP star spectra. It was found that layers exist in the stellar atmospheres considered where the Stark broadening contribution is comparable to or larger than the Doppler width.
URI: https://research.matf.bg.ac.rs/handle/123456789/955
ISSN: 13351842
Appears in Collections:Research outputs

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