J/A+A/381/507ivo://CDS.VizieR/J/A+A/381/507doi:10.26093/cds/vizier.33810507CDSKotnik-Karuza D.Friedjung M.Selvelli P.L.2002-01-29T20:52:57Z2002-01-29T21:52:49ZCDS support team

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

cds-question@unistra.frvariable-starsnovaespectroscopyFiles table1.dat and table2.dat contain the permitted and forbidden Fe II emission lines respectively which have been selected from the optical spectrum of RR Tel between 3180 and 9455{AA}. The spectrum was observed by Crawford et al. (1999, Cat. <J/A+AS/139/135>) whose corrected line fluxes and velocity widths we took for further analysis in this work. In the tables there are also values characteristic for the corresponding multiplets and lines such as multiplet numbers, term designations, level excitation potentials and quantum numbers J. The log functions of gf's, line fluxes and wavelengths are relevant for the SAC curves.2002A&A...381..507Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/381/507CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/139/135 : The Optical Spectrum of RR Tel (Crawford+ 1999)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/381/507https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/381/507http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/381/507https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/381/507https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/381/507http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/381/507GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/381/507/table1*Accepted permitted Fe II lines from the identification list of Crawford (Crawford et al., 1999, Cat. <J/A+AS/139/135>) which have been analysed in this work by the SAC methodrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIntcCorrected intensity1e-12mW.m**-2spect.line.intensityfloatLambdaLaboratory wavelength0.1nmem.wl;phys.atmol.transitionfloatMultMultiplet numberphys.atmol.levelintlog(gf)Oscillator strengthphys.atmol.wOscStrengthfloatlog(Fl3/gf)Normalized flux defined by the SAC method (Friedjung & Muratorio, 1987A&A...188..100F)phot.flux;arith.ratiofloatlog(gfl)Lower term oscillator strengthphys.atmol.wOscStrengthfloatFWHMVelocity FWHMkm/sspect.line.widthintlLower term of the multipletphys.atmol.levelcharuUpper term of the multipletphys.atmol.levelcharEPlExcitation potential of the lower leveleVphys.energy;phys.atmol.excitationfloatEPuExcitation potential of the upper leveleVphys.energy;phys.atmol.excitationfloatJuJ number of the upper levelphys.atmol.qncharJ/A+A/381/507/table2*Accepted forbidden Fe II lines from the identification list of Crawford (Crawford et al., 1999, Cat. <J/A+AS/139/135>) which have been analysed in this work by the SAC methodEPlExcitation potential of the lower leveleVphys.energy;phys.atmol.excitationfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIntcCorrected intensity1e-12mW.m**-2spect.line.intensityfloatLambdaLaboratory wavelength0.1nmem.wl;phys.atmol.transitionfloatMultMultiplet numberphys.atmol.levelintlog(gf)Oscillator strengthphys.atmol.wOscStrengthfloatlog(Fl3/gf)Normalized flux defined by the SAC method (Friedjung & Muratorio, 1987A&A...188..100F)phot.flux;arith.ratiofloatlog(gfl)Lower term oscillator strengthphys.atmol.wOscStrengthfloatFWHMVelocity FWHMkm/sspect.line.widthintlLower term of the multipletphys.atmol.levelcharuUpper term of the multipletphys.atmol.levelcharEPuExcitation potential of the upper leveleVphys.energy;phys.atmol.excitationfloatJuJ number of the upper levelphys.atmol.qnchar