Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26as..140..191d&link_type=abstract
Astronomy and Astrophysics Supplement, v.140, p.191-192
Astronomy and Astrophysics
Astrophysics
3
Atomic Data, Line: Profiles
Scientific paper
Using the semiclassical perturbation approach, we have calculated electron-, proton-, He II-, Mg II-, Si II- and Fe II-impact line widths and shifts for 189 Ca I multiplets as a function of temperature and perturber density. Perturbers selected here are the main perturbers in solar atmospheres. Obtained results have been compared with the existing theoretical and experimental data.
Dimitrijevic Milan S.
Sahal-Bréchot Sylvie
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