J/AJ/134/926ivo://CDS.VizieR/J/AJ/134/926doi:10.26093/cds/vizier.51340926CDSKim C.Yushchenko A.V.Gopka V.F.Dorokhova T.N.Musaev F.A.,Kim S.-L.Jeon Y.-B.Ibrahimov M.Tarasov A.E.2009-12-02T16:39:44Z2009-12-02T17:31:40ZCDS support team

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

cds-question@unistra.frvariable-starsspectroscopychemical-abundancesWe investigated V2314 Oph using high-resolution (R=45000) spectral observations. The atmospheric parameters were determined using iron-line abundance analysis. We derived a mean effective temperature of Teff=7510K, mean surface gravity of logg=3.30, metallicity of [Fe/H]=-0.59, and rotation velocity of vsini=38km/s. The abundances of 19 chemical elements were determined.2007AJ....134..926Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/134/926CatalogResearchIsServedByTAP VizieR generic servicerelated-toB/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/134/926https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/134/926http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/134/926https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/134/926https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/134/926http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/134/926GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/AJ/134/926/table2Iron lines in the spectrum of V2314 OphIonIron speciesphys.atmol.elementcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintWaveWavelength in Angstroms0.1nmem.wldoubleEWEquivalent width in milli-Angstroms0.1pmspect.line.eqWidthintlog(gf)Log of the oscillator strengthphys.atmol.oscStrengthfloatElowEnergy of the low leveleVphys.energy;phys.atmol.levelfloatlogNLog of the iron number abundance (logH=12)phys.abundfloatJ/AJ/134/926/table4Lines of other elements in the spectrum of V2314 OphIonIon identification code (e.g. FeI = 26.00)phys.atmol.elementfloatWaveWavelength in Angstroms0.1nmem.wldoublelog(gf)Log of the oscillator strengthphys.atmol.oscStrengthfloatElowExcitation energyeVphys.atmol.excitationfloatDlogNLog of abundance difference from solar (2)phys.abundfloatlogNLog of V2314 Oph element abundancephys.abundfloatlogNSun? Log of solar element abundance (2)phys.abundfloatnullablebld[0,1] Level of synthetic spectrum line blending in V2314 Oph (3)meta.notefloatbldSun[0,1]? Level of synthetic spectrum line blending in Sun (3)meta.notefloatnullableDepth[0,1] Synthetic spectrum line depth in V2314 Ophphys.absorption.opticalDepth;spect.linefloatDepthSun[0,1]? Synthetic spectrum line depth in Sunphot.flux.density;arith.ratiofloatnullabledlog(gf)Change of log of the abundance for atmosphere model with log(gf) shifted by -0.2dexstat.fit.paramfloatdTeffChange of log of the abundance for atmosphere model with T_eff_ shifted by +100Kstat.fit.paramfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint