Influence of Stark broadening within Be III spectral series

Details Influence of Stark broadening within Be III spectral series Influence of Stark broadening within Be III spectral series

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pobeo..75..121d&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 75, p. 121 - 124 (2003). In: Proceedings of the X

Physics

Physics Of Stars, Stellar Systems, Stellar Atmospheres: Synthetic Spectra, Beryllium

Scientific paper

Using a semiclassical perturbation method, we have calculated electron-,
proton-, and ionized helium-impact line width and shifts for 52 Be III
multiplets as a function of temperature and perturber density. The
obtained results have been used for discussion of regularities and
systematic trends along spectral series.

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