Abstract. We calculate collision strengths and thermally averaged collision strengths for electron excitation between the one hundred and forty energetically lowest levels of Fe8+. The scattering target is more elaborate than in any earlier work and large increases are found in the excitation rates among the levels of the 3s23p53d electron configuration due to resonance series that have not been considered previously. The implications for solar and stellar spectroscopy have been discussed elsewhere (Storey & Zeippen 2001). We correct some errors that were made in generating the figures given in that paper and present corrected versions. Key words. Sun: general – atomic data – Sun: UV radiation 1. Dedication Maryvonne Le Dourneuf had sta...
Energies and lifetimes are reported for the lowest 136 levels of Fe XIV, belonging to the (1s22s22p6...
We present results for the electron-impact excitation of N-like Fe as part of the RmaX network. R-m...
Aims.In this paper we report calculations for energy levels, radiative rates, collision strengths, a...
We calculate collision strengths and thermally averaged collision strengths for electron excitation ...
International audienceA new calculation of rate coefficients for electron collisional excitation of ...
We describe, and present the results of, a new large-scale R-matrix scattering calculation for the e...
Context.Absorption or emission lines of $\ion{Fe}{ii}$ are observed in many astrophysical spectra an...
New atomic calculations for Fe x are presented. They focus on the need to model the soft X-ray spect...
The distorted wave extension of the autostructure code has been used to calculate energy levels, rad...
Context. Accurate electron collisional data are required for the analysis of the Fe XIX astrophysica...
We present R-matrix results for the electron-impact excitation of Fe6+. The intermediate-coupling fr...
The EUV spectrum of $\ion{Fe}{viii}$ is reviewed, using new solar observations from the Hinode EUV...
We present new large-scale R-matrix (up to n = 4) and distorted-wave (DW, up to n = 6) scattering ca...
We present results for electron-impact excitation of F-like Fe calculated using R-matrix theory wher...
International audienceA new R-matrix calculation of rate coefficients for electron collisional excit...
Energies and lifetimes are reported for the lowest 136 levels of Fe XIV, belonging to the (1s22s22p6...
We present results for the electron-impact excitation of N-like Fe as part of the RmaX network. R-m...
Aims.In this paper we report calculations for energy levels, radiative rates, collision strengths, a...
We calculate collision strengths and thermally averaged collision strengths for electron excitation ...
International audienceA new calculation of rate coefficients for electron collisional excitation of ...
We describe, and present the results of, a new large-scale R-matrix scattering calculation for the e...
Context.Absorption or emission lines of $\ion{Fe}{ii}$ are observed in many astrophysical spectra an...
New atomic calculations for Fe x are presented. They focus on the need to model the soft X-ray spect...
The distorted wave extension of the autostructure code has been used to calculate energy levels, rad...
Context. Accurate electron collisional data are required for the analysis of the Fe XIX astrophysica...
We present R-matrix results for the electron-impact excitation of Fe6+. The intermediate-coupling fr...
The EUV spectrum of $\ion{Fe}{viii}$ is reviewed, using new solar observations from the Hinode EUV...
We present new large-scale R-matrix (up to n = 4) and distorted-wave (DW, up to n = 6) scattering ca...
We present results for electron-impact excitation of F-like Fe calculated using R-matrix theory wher...
International audienceA new R-matrix calculation of rate coefficients for electron collisional excit...
Energies and lifetimes are reported for the lowest 136 levels of Fe XIV, belonging to the (1s22s22p6...
We present results for the electron-impact excitation of N-like Fe as part of the RmaX network. R-m...
Aims.In this paper we report calculations for energy levels, radiative rates, collision strengths, a...