Abstract
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 33 Sr I multiplets for perturber densities 1013 cm-3 (for stellar plasma research) and 1015 - 1018 cm-3 (for laboratory plasma research) and temperatures T = 2 500 - 50 000 K.
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APA
Dimitrijević, M. S., & Sahal-Bréchot, S. (1996). Stark broadening of Sr i spectral lines. Astronomy and Astrophysics Supplement Series, 119(3), 529–530. https://doi.org/10.1051/aas:1996265
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