Atomic decay data for modeling the Al K lines

Details Atomic decay data for modeling the Al K lines Atomic decay data for modeling the Al K lines

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011a%26a...525a..59p&link_type=abstract

Astronomy and Astrophysics, Volume 525, id.A59

Astronomy and Astrophysics

Astrophysics

3

Atomic Data, Atomic Processes, Line: Formation, X-Rays: General

Scientific paper

Radiative and Auger decay data have been calculated for modeling the K lines of the aluminum isonuclear sequence, from Al0 up to Al11+. Level energies, transition wavelengths, radiative transition probabilities, and radiative and Auger widths were determined using Cowan's Hartree-Fock with relativistic corrections (HFR) method. Results are compared with data sets computed with the AUTOSTRUCTURE and GRASP atomic structure codes and with available experimental and theoretical values, mainly in highly ionized ions and in the solid state.
Full Tables 14 and 15 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/525/A59

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