Electron-impact excitation of H-like ions (Malespin+, 2011)

Physics – Atomic Physics

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Atomic Physics

Scientific paper

These tables contain level energies, spontaneous emission coefficients and effective collision strengths for H-like Mn, Cr, Fe, Co and Ni. The data is for the first 5 n-shells. The atomic data is for use in modelling emission from supernovae remnant plasmas, or other highly charged astrophysical sources.
A second set of atomic data is also archived, containing the photon emissivity coefficients for the strongest transitions for each of these ions, on a temperature/density grid.
The files in ADAS format are available in adas subdirectory. There are two types of data we made, one containing the description of the ion and the effective collision strengths and spontaneous emission coefficients. The other file contains the photon emissivities on a temperature/density grid of values. ADAS provides fortran routines which can read these files
(26 data files).

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