Stark broadening of spectral lines of multicharged ions of astrophysical interest. III- O VI lines.
Abstract
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.
- Publication:
-
Astronomy and Astrophysics Supplement Series
- Pub Date:
- May 1992
- Bibcode:
- 1992A&AS...93..359D
- Keywords:
-
- Charged Particles;
- Line Spectra;
- Plasma Temperature;
- Spectral Line Width;
- Stark Effect;
- Electron Impact;
- Quantum Mechanics;
- Astrophysics