J/MNRAS/490/1821ivo://CDS.VizieR/J/MNRAS/490/1821doi:10.26093/cds/vizier.74901821CDSCasamiquela L.Blanco-Cuaresma S.Carrera R.Balaguer-Nunez L.,Jordi C.Anders F.Chiappini C.Carbajo-Hijarrubia J.Aguado D.S.,del Pino A.Diaz-Perez L.Gallart C.Pancino E.2024-08-20T20:13:37Z2020-01-09T14:55:44ZCDS support team

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

cds-question@unistra.fropen-star-clusterschemical-abundancesThe study of open-cluster chemical abundances provides insights on stellar nucleosynthesis processes and on Galactic chemo-dynamical evolution. In this paper we present an extended abundance analysis of 10 species (Fe, Ni, Cr, V, Sc, Si, Ca, Ti, Mg, O) for red giant stars in 18 OCCASO clusters. This represents a homogeneous sample regarding the instrument features, method, line list and solar abundances from confirmed member stars. We perform an extensive comparison with previous results in the literature, and in particular with the Gaia FGK Benchmark stars Arcturus and mu Leo. We investigate the dependence of [X/Fe] with metallicity, Galactocentric radius (6.5kpc<RGC<11kpc), age (0.3Gyr<Age<10Gyr), and height above the plane (|z|<1000pc). We discuss the observational results in the chemo-dynamical framework, and the radial migration impact when comparing with chemical evolution models. We also use APOGEE DR14 data to investigate the differences between the abundance trends in RGC and |z| obtained for clusters and for field stars.2019MNRAS.490.1821Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/490/1821CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/458/3150 : OCCASO survey. HRV for 12 open clusters (Casamiquela+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/490/1821https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/490/1821http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/490/1821https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/490/1821https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/490/1821http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/490/1821GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/490/1821/table5 (*Cluster abundances)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/490/1821/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/490/1821/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/490/1821/table5?GETtext/xml+votable180.050000true279.635.490.0055555555555555566/1302 2436 4078 4298 6149 14175 14246 14575 14752 15396 15595 15709 24121 24522 30215 30439 31812 40696https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/490/1821?format=asciidefaultJ/MNRAS/490/1821/table2Linelist tableRefReference (1)meta.ref;pos.framecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaCentral wavelength of the line0.1nmem.wl.central;spect.linedoubleElChemical element, including ionization statephys.atmol.element;phys.atmol.ionizationcharEPExcitation potential of the transitioneVphys.atmol.excitation;phys.atmol.transitionfloatloggfOscillator strengthphys.atmol.oscStrengthfloatJ/MNRAS/490/1821/table5*Cluster abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterName of the clustermeta.id.parentcharo_FeNumber of stars used to compute Fe abundancemeta.numberint[Fe/H]Mean Fe abundancelog(Sun)phys.abund.Fe;stat.meanfloats_[Fe/H]Standard deviation of the Fe abundancelog(Sun)stat.stdev;phys.abund.Fefloato_NiNumber of stars used to compute Ni abundancemeta.numberint[Ni/H]Mean Ni abundancelog(Sun)phys.abundfloats_[Ni/H]Standard deviation of the Ni abundancelog(Sun)stat.stdev;phys.abundfloat[Ni/Fe]Mean [Ni/Fe] abundancelog(Sun)phys.abundfloats_[Ni/Fe]Standard deviation of the [Ni/Fe] abundancelog(Sun)stat.stdev;phys.abundfloato_CrNumber of stars used to compute Cr abundancemeta.numberint[Cr/H]Mean Cr abundancelog(Sun)phys.abundfloats_[Cr/H]Standard deviation of the Cr abundanceslog(Sun)stat.stdev;phys.abundfloat[Cr/Fe]Mean [Cr/Fe] abundancelog(Sun)phys.abundfloats_[Cr/Fe]Standard deviation of the [Cr/Fe] abundancelog(Sun)stat.stdev;phys.abundfloato_VNumber of stars used to compute V abundancemeta.numberint[V/H]Mean V abundancelog(Sun)phys.abundfloats_[V/H]Standard deviation of the V abundancelog(Sun)stat.stdevfloat[V/Fe]Mean [V/Fe] abundancelog(Sun)phys.abundfloats_[V/Fe]Standard deviation of the [V/Fe] abundancelog(Sun)stat.stdev;phys.abundfloato_ScNumber of stars used to compute Sc abundancemeta.numberint[Sc/H]Mean Sc abundancelog(Sun)phys.abundfloats_[Sc/H]Standard deviation of the Sc abundanceslog(Sun)stat.stdev;phys.abundfloat[Sc/Fe]Mean [Sc/Fe] abundancelog(Sun)phys.abundfloats_[Sc/Fe]Standard deviation of the [Sc/Fe] abundancelog(Sun)stat.stdev;phys.abundfloato_SiNumber of stars used to compute Si abundancemeta.numberint[Si/H]Mean Si abundancelog(Sun)phys.abundfloats_[Si/H]Standard deviation of the Si abundanceslog(Sun)stat.stdev;phys.abund.Zfloat[Si/Fe]Mean [Si/Fe] abundancelog(Sun)phys.abundfloats_[Si/Fe]Standard deviation of the [Si/Fe] abundancelog(Sun)stat.stdev;phys.abundfloato_CaNumber of stars used to compute Ca abundancemeta.numberint[Ca/H]Mean Ca abundancelog(Sun)phys.abundfloats_[Ca/H]Standard deviation of the Ca abundanceslog(Sun)stat.stdev;phys.abundfloat[Ca/Fe]Mean [Ca/Fe] abundancelog(Sun)phys.abundfloats_[Ca/Fe]Standard deviation of the [Ca/Fe] abundancelog(Sun)stat.stdev;phys.abundfloato_TiNumber of stars used to compute Ti abundancemeta.numberint[Ti/H]Mean Ti abundancelog(Sun)phys.abundfloats_[Ti/H]Standard deviation of the Ti abundanceslog(Sun)stat.stdev;phys.abund.Zfloat[Ti/Fe]Mean [Ti/Fe] abundancelog(Sun)phys.abundfloats_[Ti/Fe]Standard deviation of the [Ti/Fe] abundancelog(Sun)stat.stdev;phys.abundfloato_MgNumber of stars used to compute Mg abundancemeta.numberint[Mg/H]Mean Mg abundancelog(Sun)phys.abundfloats_[Mg/H]Standard deviation of the Mg abundanceslog(Sun)stat.stdev;phys.abundfloat[Mg/Fe]Mean [Mg/Fe] abundancelog(Sun)phys.abundfloats_[Mg/Fe]Standard deviation of the [Mg/Fe] abundancelog(Sun)stat.stdev;phys.abundfloato_ONumber of stars used to compute O abundancemeta.numberint[O/H]? Mean O abundancelog(Sun)phys.abundfloatnullables_[O/H]? Standard deviation of the O abundanceslog(Sun)stat.stdev;phys.abundfloatnullable[O/Fe]? Mean [O/Fe] abundancelog(Sun)phys.abundfloatnullables_[O/Fe]? Standard deviation of the [O/Fe] abundancelog(Sun)stat.stdev;phys.abundfloatnullableSimbadSimbad column added by the CDSmeta.ref.urlchar_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.mainJ/MNRAS/490/1821/table4Individual abundances from spectra[Ni/H]Abundance [Ni/H]phys.abundfloatInstrInstrument (2)meta.id;instrcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarIdentificator of the star (1)meta.id;meta.maincharClusterName of the clustermeta.id.parentcharONameName of the star (from WEBDA)meta.idchar[Fe/H]Abundance [Fe/H]phys.abund.Fefloate_[Fe/H]Error in [Fe/H] abundancestat.error;phys.abund.Fefloate_[Ni/H]Error in [Ni/H] abundancestat.error;phys.abundfloat[Cr/H]Abundance [Cr/H]phys.abundfloate_[Cr/H]Error in [Cr/H] abundancestat.error;phys.abundfloat[Si/H]Abundance [Si/H]phys.abundfloate_[Si/H]Error in [Si/H] abundancestat.error;phys.abundfloat[Ca/H]Abundance [Ca/H]phys.abundfloate_[Ca/H]Error in [Ca/H] abundancestat.error;phys.abundfloat[Ti/H]Abundance [Ti/H]phys.abundfloate_[Ti/H]Error in [Ti/H] abundancestat.error;phys.abundfloat[Mg/H]Abundance [Mg/H]phys.abundfloate_[Mg/H]Error in [Mg abundancestat.error;phys.abundfloat[O/H]? Abundance [O/H]phys.abundfloatnullablee_[O/H]? Error in [O/H] abundancestat.error;phys.abundfloatnullable[Sc/H]Abundance [Sc/H]phys.abundfloate_[Sc/H]Error in [Sc abundancestat.error;phys.abundfloat[V/H]Abundance [V/H]phys.abundfloate_[V/H]Error in [V/H] abundancestat.error;phys.abundfloat[Ni/Fe]Abundance [Ni/Fe]phys.abundfloate_[Ni/Fe]Error in [Ni/Fe] abundancestat.error;phys.abundfloat[Cr/Fe]Abundance [Cr/Fe]phys.abundfloate_[Cr/Fe]Error in [Cr/Fe] abundancestat.error;phys.abundfloat[V/Fe]Abundance [V/Fe]phys.abundfloate_[V/Fe]Error in [V/Fe] abundancestat.error;phys.abundfloat[Sc/Fe]Abundance [Sc/Fe]phys.abundfloate_[Sc/Fe]Error in [Sc/Fe] abundancestat.error;phys.abundfloat[Si/Fe]Abundance [Si/Fe]phys.abundfloate_[Si/Fe]Error in [Si/Fe] abundancestat.error;phys.abundfloat[Ca/Fe]Abundance [Ca/Fe]phys.abundfloate_[Ca/Fe]Error in [Ca/Fe] abundancestat.error;phys.abundfloat[Ti/Fe]Abundance [Ti/Fe]phys.abundfloate_[Ti/Fe]Error in [Ti/Fe] abundancestat.error;phys.abundfloat[Mg/Fe]Abundance [Mg/Fe]phys.abundfloate_[Mg/Fe]Error in [Mg/Fe] abundancestat.error;phys.abundfloat[O/Fe]? Abundance [O/Fe]phys.abundfloatnullablee_[O/Fe]? Error in [O/Fe] abundancestat.error;phys.abundfloatnullableSimbadNameSimbad column added by the CDSmeta.idchar