| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1779450 | New Astronomy | 2006 | 5 Pages |
Abstract
Using the modified semiempirical approach, we have considered Stark widths for 6 Cu III, 6 Zn III and 3 Se III transitions where the full semiclassical perturbation approach is not applicable in an adequate way due to the lack of reliable atomic data. Results are obtained as a function of temperature, for perturber density of 1017 cm−3. Calculated results have been used to consider the influence of Stark broadening for A type star and DB white dwarf atmospheric conditions.
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Authors
Z. Simić, M.S. Dimitrijević, L.Č. Popović, M.D. Dačić,