Effective collision strengths for C II

DOI

The effective collision strengths are presented in this table for all transitions among the lowest 30 fine-structure levels belonging to the 2s^2^2p, 2s2p^2^, 2p^3^, 2s2p3s, 2s^2^3l (l=s,p,d) and 2s^2^4l (l=s,p,d,f) configurations of C II. The effective collision strengths have been calculated using the R-matrix method. Each fine-structure level is assigned an index number in Table 1 of the manuscript ranging from 1 to 30. These index values are used here in Table 2 to refer to particular transitions, eg. Index 2-8 denotes the transition 2s^2^2p 2PO(J=3/2) - 2s2p^2^ 3SE(J=1/2). The effective collision strengths for each transition are presented in rows for a number of electron temperatures ranging from log10(T)=3.00 to log10(T)=5.50.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34320731
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/432/731
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/432/731
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/432/731
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/432/731
Provenance
Creator Wilson N.J.; Bell K.L.; Hudson C.E.
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