Stark broadening of Si V (Ben Nessib+, 2004)

Details Stark broadening of Si V (Ben Nessib+, 2004) Stark broadening of Si V (Ben Nessib+, 2004)

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34230397b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/423/397. Originally published in: 2004A&A...423..397B

Physics

Atomic Physics

Atomic Physics

Scientific paper

Using a semiclassical perturbation approach, we have obtained Stark broadening parameters for 16 Si V multiplets using atomic data calculated ab initio with the SUPERSTRUCTURE code. In order to complete Stark broadening data for the most important charged perturbers in stellar atmospheres, Stark broadening parameters for proton-, He II-, and Si II-impact line widths and shifts are also presented. Results have been obtained for an electron density of 1017cm-3 as a function of temperature. Moreover, we have performed the same calculations with oscillator strengths calculated within the Coulomb approximation.
(2 data files).

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