In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 52, no. 3
Z. Simić - M.s. Dimitrijević - S. Sahal-Bréchot - N. Sakan
Details:
Year, pages: 2022, 35 - 43
Language: eng
Keywords:
Atomic data, Spectral lines, A type stars
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2022/Vol_52/No_3/pp35-43_abstract.html
About article:
Stark broadening parameters for four Sn III spectral line obtained by using semiclassical perturbation approach and Stark widths for this transitions obtained by using modified semiempirical approach have been compared with available experimental and semiempirical data and used for the consideration of the influence of the Stark broadening effect in A type stellar atmospheres.
How to cite:
ISO 690:
Simić, Z., Dimitrijević, M., Sahal-Bréchot, S., Sakan, N. 2022. On the Stark broadening parameters of Sn III spectral lines. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 52, no.3, pp. 35-43. 1335-1842. DOI: https://doi.org/10.31577/caosp.2022.52.3.35
APA:
Simić, Z., Dimitrijević, M., Sahal-Bréchot, S., Sakan, N. (2022). On the Stark broadening parameters of Sn III spectral lines. Contributions of the Astronomical Observatory Skalnaté Pleso, 52(3), 35-43. 1335-1842. DOI: https://doi.org/10.31577/caosp.2022.52.3.35
About edition:
Publisher: Astronomical Institute, Slovak Academy of Sciences
Published: 1. 12. 2022
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