Aims. In this paper we report on calculations for energy levels, radiative rates, collision strengths, and effective collision strengths for transitions among the lowest 25 levels of the n ≤ 5 configurations of H-like Ar xvii
We calculate in this work quantum Stark broadening, radiative atomic data (energy levels, radiative ...
Electron impact excitation collision strengths are calculated for all transitions among 113 levels o...
International audienceWe present in this work Stark broadening calculations for 12 Ar XII and 12 Ar ...
Aims. In this paper we report on calculations for energy levels, radiative rates, collision strength...
Context. Many observed emission lines from space missions are due to highly charged H-like ions. An ...
Aims. In this paper we report on calculations of energy levels, radiative rates, oscillator strength...
Context. Many observed emission lines from space missions are due to highly charged H-like ions. An ...
We report calculations of energy levels, radiative rates, collision strengths and effective collisio...
Aims. In this paper we report calculations for energy levels, radiative rates, and electron impact e...
Energies for the lowest 49 levels among the 1s2 and 1s$n\ell$ ($n = 2{-}5$) configurations of Ar XVI...
Aims. This work reports on radiative transition rates and electron impact excitation collision stren...
Context. Emission from Ar III is seen in planetary nebulae, in H II regions, and from laboratory p...
Aims.In this paper we report calculations for energy levels, radiative rates, collision strengths, a...
Energy levels and radiative rates for transitions among the lowest 97 fine-structure levels belongin...
Abstract: Collision strengths for transitions among the n = 5 levels of AI XI11 have been computed i...
We calculate in this work quantum Stark broadening, radiative atomic data (energy levels, radiative ...
Electron impact excitation collision strengths are calculated for all transitions among 113 levels o...
International audienceWe present in this work Stark broadening calculations for 12 Ar XII and 12 Ar ...
Aims. In this paper we report on calculations for energy levels, radiative rates, collision strength...
Context. Many observed emission lines from space missions are due to highly charged H-like ions. An ...
Aims. In this paper we report on calculations of energy levels, radiative rates, oscillator strength...
Context. Many observed emission lines from space missions are due to highly charged H-like ions. An ...
We report calculations of energy levels, radiative rates, collision strengths and effective collisio...
Aims. In this paper we report calculations for energy levels, radiative rates, and electron impact e...
Energies for the lowest 49 levels among the 1s2 and 1s$n\ell$ ($n = 2{-}5$) configurations of Ar XVI...
Aims. This work reports on radiative transition rates and electron impact excitation collision stren...
Context. Emission from Ar III is seen in planetary nebulae, in H II regions, and from laboratory p...
Aims.In this paper we report calculations for energy levels, radiative rates, collision strengths, a...
Energy levels and radiative rates for transitions among the lowest 97 fine-structure levels belongin...
Abstract: Collision strengths for transitions among the n = 5 levels of AI XI11 have been computed i...
We calculate in this work quantum Stark broadening, radiative atomic data (energy levels, radiative ...
Electron impact excitation collision strengths are calculated for all transitions among 113 levels o...
International audienceWe present in this work Stark broadening calculations for 12 Ar XII and 12 Ar ...
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