Ni XXV energy levels and radiative rates

DOI

We report calculations of energy levels and radiative rates for 1300 fine-structure levels generated from 189 configurations of Be-like Nickel. The General Purpose Relativistic Atomic Structure Program (GRASP2), developed by the I.P. Grant group in 1989 and partly improved by our group, is adopted in the calculations of energy levels and radiative rates. Our calculations are compared with those of other numerical methods and experiments so that their accuracy can be assessed. Additionally, the wavelengths, oscillator strengths, and radiative rates (for a given radiative rate and level structure, it is then easy to derive the line strength) a re reported for all electric dipole (E1), electric quadrupole (E2), magnetic dipole (M1) and magnetic quadrupole (M2) transitions among these levels. Finally, the lifetimes of all excited levels are reported.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34881155
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/488/1155
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/488/1155
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/488/1155
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/488/1155
Provenance
Creator Duan B.; Bari M.A.; Zhong J.Y.; Yan J.; Li M.Y.; Zhang J.
Publisher CDS
Publication Year 2008
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