J/A+A/430/255ivo://CDS.VizieR/J/A+A/430/255doi:10.26093/cds/vizier.34300255CDSYushchenko A.Gopka V.Goriely S.Musaev F.Shavrina A.Kim C.,Woon Kang Y.Kuznietsova J.Yushchenko V.2006-09-13T06:29:15Z2006-09-13T06:25:40ZCDS support team

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

cds-question@unistra.frvariable-starschemical-abundancesspectroscopyWe report the abundance determination in the atmosphere of the bright halo star HD 221170. The spectra were taken with the Terskol Observatory's 2.0-m telescope with a resolution R=45000 and signal-to-noise ratio up to 250 in the wavelength region 3638-10275{AA}. The abundances of 43 chemical elements were determined with the method of spectrum synthesis.2005A&A...430..255Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/430/255CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/430/255https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/430/255http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/430/255https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/430/255https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/430/255http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/430/255GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/430/255/table1Iron lines in the spectrum of HD 221170recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength0.1nmem.wldoubleIonIonphys.atmol.ionStagecharEWEquivalent width0.1pmspect.line.eqWidthfloatloggfOscillator strengthphys.atmol.oscStrengthfloatElowEnergy of lower leveleVphys.energy;phys.atmol.levelfloatlogNAbundance, in logN(H)=12 scalephys.abundfloatJ/A+A/430/255/table2Lines of other elements in the spectrum of HD 221170logNS? Sun abundance (in logN(H)=12 scale)phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIon number (e.g. 26.00 = Fe I)meta.id;meta.mainfloatlambdaWavelength0.1nmem.wldoubleloggfOscillator strengthphys.atmol.oscStrengthfloatn_loggf[ab] Note on loggf (1)meta.notecharElowEnergy of lower leveleVphys.energy;phys.atmol.levelfloatl_AbunLimit flag on DlogNmeta.code.errorcharAbunAbundance of ion (relative to Sun, log scale)log(Sun)phys.abundfloatl_logNLimit flag on logNmeta.code.errorcharlogNHD 221170 abundance (in logN(H)=12 scale)(2)phys.abundfloatBlend? HD 221170 level of blending (1=clean line)meta.notefloatnullableBlendS? Sun level of blending (1=clean line)meta.notefloatnullableDepth? HD 221170 depth in synthetic spectra (2)phot.flux.density;arith.ratiofloatnullableDepthS? Sun depth in synthetic spectraphot.flux.density;arith.ratiofloatnullabledAbG? Abundance change with logg (+0.2)log(Sun)stat.errorfloatnullabledAbT? Abundance change with Teff (+100K)log(Sun)stat.errorfloatnullable