Na-like iso-electronic sequence

DOI

We present our calculated data including energy levels, radiative decay rates and effective collision strengths for all the transitions among the 32 fine-structure levels arising from the 18 lowest LS states of Na-like iso-electronic sequence, i.e. those with configurations: 2p(6)3l (l=s,p,d); 2p(6)4l (l=s,p,d,f); 2p(6)5l (l=s,p,d,f,g); 2p(6)6l (l=s,p,d,f,g,h). The effective collision strengths at 13 temperatures ranging from 2x10^2(q+1)^2 to 2x10^6(q+1)^2 K, where q is the residual charge of ions, i.e. Z-11, have been calculated using the ICFT R-matrix method. The data format adopts ADAS adf04 format, see the file at website http://www.adas.ac.uk/man/appxa-04.pdf

Identifier
DOI http://doi.org/10.26093/cds/vizier.35001263
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/500/1263
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/500/1263
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/500/1263
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/500/1263
Provenance
Creator Liang G.Y.; Whiteford A.D.; Badnell N.R.
Publisher CDS
Publication Year 2009
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