Atomic data for X-ray lines of FeVIII and FeIX

DOI

The distorted wave extension of the autostructure code has been used to calculate energy levels, radiative transition probabilities and collisional excitation rates of Fe VIII and Fe IX up to n=6 for Fe IX and n=7 for Fe VIII. We have compared some of the data with previous calculations, finding overall agreement for radiative transition rates, but interesting differences for some collisional data. *********** * * Sorry, but the author(s) never supplied the tabular material * announced in the paper * * ************

Identifier
DOI http://doi.org/10.26093/cds/vizier.35370022
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/537/A22
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/537/A22
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/537/A22
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/537/A22
Provenance
Creator O'Dwyer B.; Del Zanna G.; Badnell N.R.; Mason H.E.; Storey P.J.
Publisher CDS
Publication Year 2012
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Physics