On the Stark broadening of the four times ionized silicon spectral lines

Details On the Stark broadening of the four times ionized silicon spectral lines On the Stark broadening of the four times ionized silicon spectral lines

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pobeo..76..167b&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 76, p. 167 - 170 (2003). In: IV Serbian Conferenc

Astronomy and Astrophysics

Astronomy

Stark Broadening, Spectral Lines, Silicon

Scientific paper

Using a semiclassical perturbation approach, we have compared Stark broadening parameters for 16 Si V multiplets calculated with oscillator strengths obtained with the SUPERSTRUCTURE code and within the Coulomb approximation. In order to complete Stark broadening data for most important charged perturbers in stellar atmospheres, Stark broadening parameters for proton-, He II-, and Si II-impact line widths and shifts are presented also.

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