Effective collision strengths for Al III

DOI

Effective collision strengths are presented for all the transitions among the 17 fine-structure levels arising from the 10 lowest LS states of Al III, 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). The effective collision strengths have been calculated using the R-matrix method. Each fine-structure level is assigned an index number ranging from 1 to 17, which are noted in the file 'j-index.dat'. The index values are used here in Table 7 to refer to particular transitions, eg. Index 1-3 denotes the 2p(6)3s 2SE(J=1/2) -- 2p(6)3p 2PO(J=3/2) transition.The effective collision strengths for each transition are presented for electron temperatures ranging from log10(T)=3.6 to log10(T)=5.60 in steps of 0.1.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34361131
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/436/1131
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/436/1131
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/436/1131
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/436/1131
Provenance
Creator Hudson C.E.; Bell K.L.
Publisher CDS
Publication Year 2005
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