Stark broadening parameters for Cu III, Zn III and Se III lines in laboratory and stellar plasma

Details Stark broadening parameters for Cu III, Zn III and Se III lines in laboratory and stellar plasma Stark broadening parameters for Cu III, Zn III and Se III lines in laboratory and stellar plasma

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006newa...12..187s&link_type=abstract

New Astronomy, Volume 12, Issue 3, p. 187-191.

Astronomy and Astrophysics

Astronomy

6

32.70.Jz, 95.30.Ky, 97.10Ex

Scientific paper

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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