R-matrix calculations of electron impact excitations have been done for several isoelectronic sequences under the program of the Atomic Processes for Astrophysical Plasmas network in the United Kingdom. The intermediate-coupling framework transformation R-matrix approach was used to generate data in this program since it is less resource (time/memory) demanding than the full Breit-Pauli R-matrix method, without reduction of accuracy. A detailed accuracy assessment was done for four/five/six selected ions spanning the isoelectronic sequence, which provides insight into the behavior of the whole sequence of ions. For each ion, we adopted the following procedure: First, the target structure was assessed by comparing the calculated level energi...
Context. Emission from Ar III is seen in planetary nebulae, in H II regions, and from laboratory p...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for reliable diagno...
We present results for the electron-impact excitation of N-like Fe as part of the RmaX network. R-ma...
R-matrix calculations of electron impact excitations have been done for several isoelectronic sequen...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for relia...
Emission lines from ions in the Mg-like iso-electronic sequence can be used as reliable diagnostics ...
We have carried-out parallel intermediate-coupling frame transformation R-matrix calculations for el...
We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained...
We present results for the electron-impact excitation of F-like ions from Ne+ to Kr27+ using an R-ma...
Context. Astrophysical plasma codes are built on atomic databases. In the current atomic databases, ...
We have carried-out parallel intermediate-coupling frame transformation R-matrix calculations for el...
We present results for the outer-shell electron-impact excitation of all Na-like ions from Mg+ to Kr...
We present results for the electron-impact excitation of all Li-like ions from Be+ to Kr33+ which we...
Plasma models built on extensive atomic data are essential to interpret the observed X-ray spectra. ...
Context. Emission from Ar III is seen in planetary nebulae, in H II regions, and from laboratory p...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for reliable diagno...
We present results for the electron-impact excitation of N-like Fe as part of the RmaX network. R-ma...
R-matrix calculations of electron impact excitations have been done for several isoelectronic sequen...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for relia...
Emission lines from ions in the Mg-like iso-electronic sequence can be used as reliable diagnostics ...
We have carried-out parallel intermediate-coupling frame transformation R-matrix calculations for el...
We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained...
We present results for the electron-impact excitation of F-like ions from Ne+ to Kr27+ using an R-ma...
Context. Astrophysical plasma codes are built on atomic databases. In the current atomic databases, ...
We have carried-out parallel intermediate-coupling frame transformation R-matrix calculations for el...
We present results for the outer-shell electron-impact excitation of all Na-like ions from Mg+ to Kr...
We present results for the electron-impact excitation of all Li-like ions from Be+ to Kr33+ which we...
Plasma models built on extensive atomic data are essential to interpret the observed X-ray spectra. ...
Context. Emission from Ar III is seen in planetary nebulae, in H II regions, and from laboratory p...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for reliable diagno...
We present results for the electron-impact excitation of N-like Fe as part of the RmaX network. R-ma...