J/PASJ/59/1127ivo://CDS.VizieR/J/PASJ/59/1127doi:10.26093/cds/vizier/bj-1v-137CDSTakeda Y.Taguchi H.Yoshioka K.Hashimoto O.Aikawa T.Kawanomoto S.2026-03-17T20:04:49Z2009-02-22T07:27:05ZCDS support team

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

cds-question@unistra.frsupergiant-starschemical-abundancesA detailed non-LTE study on the abundances of C, N, O, S, and Zn was carried out for five F-G supergiants of suspected post-AGB candidates with IR excesses (HD 112374, HD 148743, HD 161796, HD 163506, and HD 187203), since these volatile elements can provide the key to inferring the original metallicity as well as an evolution-induced change due to mixing, given that they are free from depletion caused by dust-gas separation.2007PASJ...59.1127Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/59/1127CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASJ/59/1127https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASJ/59/1127http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASJ/59/1127https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASJ/59/1127https://vizier.iucaa.in/viz-bin/votable?-source=J/PASJ/59/1127http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASJ/59/1127GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/PASJ/59/1127/table6Averaged abundances and sensitivities to atmospheric parameters[X/Fe]Relative abundance to Fephys.abund.FefloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElElementphys.atmol.elementcharHDStar HD numbermeta.id;meta.mainint[Fe/H]Metallicityphys.abund.Zfloat<AX>Final (averaged) logarithmic abundance for element X with the usual normalization of AH=12 (1)phys.abundfloate_<AX>? Standard deviation in deriving <AX>stat.errorfloatnullable[X/H]Relative abundance in comparison to the Sun (2)log(Sun)phys.abundfloat[X/Zn]Relative abundance to Znphys.abundfloatdT-Delta value of <AX> with temperature change (3)stat.stdevfloatdT+Delta value of <AX> with temperature change (3)stat.stdevfloatdg-Delta value of <AX> with gravity change (3)stat.stdevfloatdg+Delta value of <AX> with gravity change(3)stat.stdevfloatdv-Delta value of <AX> with turbulence change (3)stat.stdevfloatdv+Delta value of <AX> with turbulence change (3)stat.stdevfloatJ/PASJ/59/1127/table2Line data and equivalent widths of Fe lines along with the resulting abundances corresponding to the final atmospheric parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDStar HD numbermeta.id;meta.mainintIonIon codemeta.code;phys.atmol.ionStagefloatlambdaLine wavelength0.1nmem.wl;spect.linedoubleEPExcitation potentialeVphys.atmol.excitationfloatloggfOscillator strengthphys.atmol.oscStrengthfloatEW? Equivalent width0.1pmspect.line.eqWidthfloatnullableAbund? Abundance (AH=12)phys.abundfloatnullableJ/PASJ/59/1127/table4Adopted atomic data of spectral linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRegionRegion (1)meta.notecharIonIon designation (1)meta.id;phys.atmol.ionStagecharRMTMultiplet number (1)meta.id;meta.maincharLine? Line (1)0.1nmmeta.id;spect.lineintnullablelambdaWavelength (1)0.1nmem.wldoubleEP? Excitation potential (1)eVphys.atmol.excitationfloatnullableloggfOscillator strength (1)phys.atmol.oscStrengthfloatGammar? Radiation damping constant (log(gamma_red_))phys.dampingfloatnullablen_Gammar[*] Note (2)meta.notecharGammas? Stark damping width per electron density at 10^4^K, log(gamma_e_/N_e_)spect.line.broad.Starkfloatnullablen_Gammas[*] Note (2)meta.notecharGammaw? van der Waals damping width per hydrogen density at 10^4^K, log(gamma_w_/N_H_)phys.densityfloatnullablen_Gammaw[*] Note (2)meta.notecharJ/PASJ/59/1127/table5Line-by-line equivalent widths, abundances, and non-LTE correctionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDStar HD numbermeta.id;meta.mainintRegionRegionmeta.notecharLineLine0.1nmmeta.id;spect.lineintEW? Equivalent width0.1pmspect.line.eqWidthfloatnullableAbund? Abundancephys.abundfloatnullablen_Abund[)] Note (1)meta.notecharDN? Non-LTE correctionarith.factorfloatnullable