Radiative oscillator strengths for 103 lines arising from 5s5p6s, 5s5p5d and 5p3 configurations of Sn II and lifetimes corresponding to several levels of these configurations have been calculated. These values were obtained in intermediate coupling (IC) and using ab initio relativistic Hartree-Fock (HFR) calculations. We use the standard method of least square fitting of experimental energy levels for the IC calculations by means of computer codes from Cowan
Transition probabilities have been calculated for $\Delta n = 0$ and $\Delta n = 1$ transitions conn...
International audienceOscillator strengths have been calculated for the transitions depopulating lev...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Radiative oscillator strengths for 103 lines arising from 5s5p6s, 5s5p5d and 5p3 configurations of ...
Radiative oscillator strengths for 103 lines arising from 5s5p6s, 5s5p5d and 5p³ configurations of S...
Radiative transition probabilities and oscillator strengths for 164 lines arising from 5s²ns, 5s²np,...
Theoretical values of oscillator strengths and transition probabilities for 306 spectral lines arisi...
Transition probabilities and oscillator strengths of 382 lines with astrophysical interest arising f...
Semi-empirical weighted oscillator strengths (gf) and lifetimes presented in this work for all exper...
The weighted oscillator strengths (gf) and lifetimes for S VIII presented in this work were obtained...
The weighted oscillator strengths gf and the lifetimes for S XIV presented in this work have been ca...
The weighted oscillator strengths (gf) and the lifetimes presented in this work were carried out in ...
The weighted oscillator strengths gf and the lifetimes for S XIV presented in this work have been ca...
The weighted oscillator strengths (gf) and the lifetimes presented in this work were carried out in ...
The weighted oscillator strengths (gf) and the lifetimes for Si IV presented in this work were carri...
Transition probabilities have been calculated for $\Delta n = 0$ and $\Delta n = 1$ transitions conn...
International audienceOscillator strengths have been calculated for the transitions depopulating lev...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Radiative oscillator strengths for 103 lines arising from 5s5p6s, 5s5p5d and 5p3 configurations of ...
Radiative oscillator strengths for 103 lines arising from 5s5p6s, 5s5p5d and 5p³ configurations of S...
Radiative transition probabilities and oscillator strengths for 164 lines arising from 5s²ns, 5s²np,...
Theoretical values of oscillator strengths and transition probabilities for 306 spectral lines arisi...
Transition probabilities and oscillator strengths of 382 lines with astrophysical interest arising f...
Semi-empirical weighted oscillator strengths (gf) and lifetimes presented in this work for all exper...
The weighted oscillator strengths (gf) and lifetimes for S VIII presented in this work were obtained...
The weighted oscillator strengths gf and the lifetimes for S XIV presented in this work have been ca...
The weighted oscillator strengths (gf) and the lifetimes presented in this work were carried out in ...
The weighted oscillator strengths gf and the lifetimes for S XIV presented in this work have been ca...
The weighted oscillator strengths (gf) and the lifetimes presented in this work were carried out in ...
The weighted oscillator strengths (gf) and the lifetimes for Si IV presented in this work were carri...
Transition probabilities have been calculated for $\Delta n = 0$ and $\Delta n = 1$ transitions conn...
International audienceOscillator strengths have been calculated for the transitions depopulating lev...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...