On the Stark broadening parameters of Sn III spectral lines
Abstract
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.
- Publication:
-
Contributions of the Astronomical Observatory Skalnate Pleso
- Pub Date:
- December 2022
- DOI:
- 10.31577/caosp.2022.52.3.35
- Bibcode:
- 2022CoSka..52c..35S
- Keywords:
-
- Atomic data;
- Spectral lines;
- A type stars