S V effective collision strengths

DOI

Effective collision strengths are presented in this table for all the transitions among the 26 fine-structure levels arising from the 14 lowest LS states of S V, i.e. those with configurations: (2p^6^)3s^2^, 3s3p, 3p^2^, 3s3d, 3s4s, 3p3d. 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 26, which are noted in the paper as Table 5. The index values are used here in Table 7 to refer to particular transitions, eg. Index 2-8 denotes the 2p(6)3s3p 3PO(J=0)- 2p(6)3p^2^ 3PE(J=1) transition. The effective collision strengths for each transition are presented for electron temperatures ranging from log10(T)=4.0 to log10(T)=6.0 in steps of 0.1.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34521113
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/452/1113
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/452/1113
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/452/1113
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/452/1113
Provenance
Creator Hudson C.E.; Bell K.L.
Publisher CDS
Publication Year 2006
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