J/AZh/84/429ivo://CDS.VizieR/J/AZh/84/429CDSMishenina T.V.Gorbaneva T.I.Bienayme O.Soubiran C.Kovtyukh V.V.,Orlova L.F.2017-12-06T07:37:52Z2008-05-31T08:01:07ZCDS support team

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

cds-question@unistra.frgiant-starschemical-abundancesWe have determined the atmospheric abundances of Y, Ba, La, Ce, Pr, Nd, and Eu for a sample of 171 giants selected as clump giants with metallicities [Fe/H] between 0.7 and 0.3dex, based on photometric criteria. In our analysis, we assumed local thermodynamic equilibrium and fit the parameters of model atmospheres to high-resolution (R=42000) echelle spectra with high signal-to-noise ratios. The Ba and Eu abundances were derived using synthetic spectra, including hyperfine structure. We find no significant difference in the abundances of s-or r-process neutron-capture elements between clump giants and ascending-branch giants selected by us earlier. We also analyze the relation between the abundances of neutron-capture elements and [Fe/H].2007AZh....84..429Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/84/429CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AZh/77/96 : Abundances in Hyades red giants (Boyarchuk+, 2000)J/AZh/81/658 : Equivalent widths of 9 barium stars (Antipova+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/84/429https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/84/429http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/84/429https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AZh/84/429https://vizier.iucaa.in/viz-bin/votable?-source=J/AZh/84/429http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AZh/84/429GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AZh/84/429/table1 (HD numbers, Teff, logg, evolutionary stages (ES), [Fe/H], and [A/Fe])https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AZh/84/429/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/AZh/84/429/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AZh/84/429/table1?GETtext/xml+votable180.050000true8.147858120.29431640.0055555555555555566/140 166 210 327 341 377 428 915 1249 1819 1960 1998 2014 2202 2229 2324 2433 2440 2541 2828 3026 3094 3335 3418 3619 3755 4051 4090 4794 4969 4985 5059 5245 5286 5589 5789 5815 5950 5983 6120 6166 6203 6251 6334 6361 6493 6827 6933 7006 7039 7113 7177 7320 7337 7422 7466 7487 7542 7771 7836 7927 8080 8536 8626 9337 10184 10256 10354 10632 10817 11659 11734 12186 12208 12995 13333 13458 13643 13731 14013 14109 14220 14604 14693 15303 15355 15363 15715 15730 15995 16013 16023 16035 16056 16150 16895 17061 17159 17573 17656 17731 17764 17852 18802 18972 19718 19799 19868 20137 20208 20893 20973 21174 21273 21286 21423 21469 21477 21572 21612 21738 21768 21829 21940 22108 22199 22293 22360 22518 22932 23230 23533 23538 23539 23547 23753 23843 24262 25571 25608 26562 26704 27014 27076 27386 27604 28104 28276 28436 28487 28660 29391 29712 30735 31444 32045 32096 32328 32348 32509 36714 40355 40588 40618 40644 44333 44347 48816 48852 48943 48980https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AZh/84/429?format=asciiOpticaldefaultJ/AZh/84/429/table1HD numbers, Teff, logg, evolutionary stages (ES), [Fe/H], and [A/Fe]HDHD numbermeta.id;meta.mainintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeffEffective temperatureKphys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloatESEvolutionnary stage, as CL = clump giant or RGB = ascending-giant branchsrc.classchar[Fe/H]Metallicitylog(Sun)phys.abund.Zfloat[Y/Fe]? Y (Z=39) abundance, relative to Felog(Sun)phys.abund.Yfloatnullable[Ba/Fe]? Ba (Z=56) abundance, relative to Felog(Sun)phys.abundfloatnullable[La/Fe]? La (Z=57) abundance, relative to Felog(Sun)phys.abund.Xfloatnullable[Ce/Fe]? Ce (Z=58) abundance, relative to Felog(Sun)phys.abundfloatnullable[Pr/Fe]? Pr (Z=59) abundance, relative to Felog(Sun)phys.abund.Xfloatnullable[Nd/Fe]? Nd (Z=60) abundance, relative to Felog(Sun)phys.abundfloatnullable[Eu/Fe]? Eu (Z=63) abundance, relative to Felog(Sun)phys.abundfloatnullableSimbadSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.main