Stark broadening of spectral lines of multicharged ions of astrophysical interest. III - O VI lines

Details Stark broadening of spectral lines of multicharged ions of astrophysical interest. III - O VI lines Stark broadening of spectral lines of multicharged ions of astrophysical interest. III - O VI lines

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...93..359d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 93, no. 2, May 1992, p. 359-371. Research supported by Obser

Astronomy and Astrophysics

Astrophysics

29

Charged Particles, Line Spectra, Plasma Temperature, Spectral Line Width, Stark Effect, Electron Impact, Quantum Mechanics

Scientific paper

A semiclassical approach has been used to calculate electron-, proton-,
and ionized helium-impact line widths and shifts for 30 O VI multiplets.
This comprehensive set of data has been used for the investigation of
Stark broadening parameter regularities within spectral series.

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