A comprehensive study of relativistic and resonance effects in electron impact excitation of (e+Fe XVII) is carried out using the BPRM method in the relativistic close coupling approximation. Two sets of eigenfunction expansions are employed; first, up to the n = 3 complex corresponding 37 fine-structure levels (37CC) from 21 LS terms; second, up to the n = 4 corresponding to 89 fine-structure levels (89CC) from 49 LS terms. In contrast to previous works, the 37CC and the 89CC collision strengths exhibit considerable differences. Denser and broader resonances due to n = 4 are present in the 89CC results both above and {\it below} the 37 thresholds, thus significantly affecting the collision strengths for the primary X-ray and EUV transition...
We present results for electron-impact excitation of F-like Fe calculated using R-matrix theory wher...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
Aims.In this paper we report calculations for energy levels, radiative rates, collision strengths, a...
Extensive calculations are reported for electron collision strengths, rate coefficients, and transit...
Ab initio theoretical calculations are reported for the electric (El) dipole allowed and intercombin...
We present results for electron-impact excitation of F-like Fe calculated using R-matrix theory wher...
Sodium-like Fe XVI is observed in collisionally ionized plasmas such as stellar coronae and coronal ...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
Context.Absorption or emission lines of $\ion{Fe}{ii}$ are observed in many astrophysical spectra an...
We present results for the electron-impact excitation of N-like Fe as part of the RmaX network. R-ma...
We have carried out a 204-level close-coupling (CC) calculation for B-like Fe using the R-matrix met...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
Energy levels and radiative rates for transitions among the lowest 97 fine-structure levels belongin...
Radiative transitions for photo-excitations and de-excitations in Fe XXII are studied in the relativ...
Context. Accurate electron collisional data are required for the analysis of the Fe XIX astrophysica...
We present results for electron-impact excitation of F-like Fe calculated using R-matrix theory wher...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
Aims.In this paper we report calculations for energy levels, radiative rates, collision strengths, a...
Extensive calculations are reported for electron collision strengths, rate coefficients, and transit...
Ab initio theoretical calculations are reported for the electric (El) dipole allowed and intercombin...
We present results for electron-impact excitation of F-like Fe calculated using R-matrix theory wher...
Sodium-like Fe XVI is observed in collisionally ionized plasmas such as stellar coronae and coronal ...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
Context.Absorption or emission lines of $\ion{Fe}{ii}$ are observed in many astrophysical spectra an...
We present results for the electron-impact excitation of N-like Fe as part of the RmaX network. R-ma...
We have carried out a 204-level close-coupling (CC) calculation for B-like Fe using the R-matrix met...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
Energy levels and radiative rates for transitions among the lowest 97 fine-structure levels belongin...
Radiative transitions for photo-excitations and de-excitations in Fe XXII are studied in the relativ...
Context. Accurate electron collisional data are required for the analysis of the Fe XIX astrophysica...
We present results for electron-impact excitation of F-like Fe calculated using R-matrix theory wher...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
Aims.In this paper we report calculations for energy levels, radiative rates, collision strengths, a...