Semi-Classical Impact Stark Shift Calculations of Singly-Ionized Carbon, Nitrogen and Oxygen Spectral Lines
Résumé
Using the semiclassical approach by Sahal-Bréchot [Astron. Astrophys. 1, 91 (1969), ibid. 2, 322 (1969)], we have calculated Stark shifts for CII, NII and OII spectral lines. The needed oscillator strengths have been obtained from the sophisticated atomic structure data base "TOPbase". Then we have compared our results with available experimental ones and with other theoretical results. We give also new values of Stark shifts.