J/A+AS/119/99ivo://CDS.VizieR/J/A+AS/119/99CDSQuinet P.Le Dourneuf M.1997-12-09T18:19:29Z1997-12-09T19:19:26ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fratomic-physicsNew radiative transition probabilities have been calculated for forbidden lines of astrophysical interest in Ni I and Ni II. The accuracy of the transition probability scales is established on the basis of two independent calculations performed with the approximately relativistic Hartree-Fock (HFR) and SUPERSTRUCTURE (SST) codes. Both physical models take into account the most important configuration interaction (CI) and relativistic effects.1996A&AS..119...99Qhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/119/99CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/119/99https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/119/99http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/119/99https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/119/99https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/119/99http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/119/99GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/119/99/table7Radiative transition probabilities, Aki in s-1, as obtained with HFR and SST for forbidden lines of Ni I.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMultipletMultiplet designationphys.atmol.levelcharJ-J'J-J'meta.id;phys.atmol.transitioncharLambdaPredicted wavelengths from observed energy levels: see note (1)0.1nmem.wl.effectivedoubleTypeType of transitionmeta.code;phys.atmol.transitioncharAki(HFR)HFR transition probabilitiess**-1phys.atmol.transProbdoublen_Aki(HFR)[*] Comment on the HFR A-value: see note (2)meta.notecharAki(SST)SST transition probabilitiess**-1phys.atmol.transProbdoubleJ/A+AS/119/99/table8Radiative transition probabilities, Aki in s-1, as obtained with HFR and SST for forbidden lines of Ni II.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMultipletMultiplet designationphys.atmol.levelchar2J-2J'2J-2J'phys.atmol.qncharLambdaPredicted wavelengths from observed energy levels: see note (1)0.1nmem.wl.effectivedoublen_Lambda[+] Comment on the wavelength: see note (2)meta.notecharTypeType of transitionmeta.code;phys.atmol.transitioncharAki(HFR)HFR transition probabilitiess**-1phys.atmol.transProbdoublen_Aki(HFR)[*] Comment on the HFR A-value: see note (3)meta.notecharAki(SST)SST transition probabilitiess**-1phys.atmol.transProbdouble