Stark broadening of spectral lines of multicharged ions of astrophysical interest. VIII - S VI lines

Details Stark broadening of spectral lines of multicharged ions of astrophysical interest. VIII - S VI lines Stark broadening of spectral lines of multicharged ions of astrophysical interest. VIII - S VI lines

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as..100...91d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 100, no. 1, p. 91-101.

Astronomy and Astrophysics

Astrophysics

10

Cosmic Plasma, Molecular Ions, Spectral Line Width, Spectrum Analysis, Stark Effect, Astronomical Spectroscopy, Electron Impact, Molecular Energy Levels, Opacity

Scientific paper

Electron-impact full halfwidths for 21 S VI multiplets of interest for stellar opacities calculations were calculated using the semiclassical-perturbation formalism developed by Sahal-Brechot (1969). In addition, Stark-broadening parameters due to proton impacts and He-III impacts were calculated. A table is presented listing the results for Stark broadening parameters for S VI multiplets.

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