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<ri:Resource created="2014-04-29T07:56:50Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Oxygen abundances in nearby FGK stars</title><shortName>J/ApJ/764/78</shortName><identifier>ivo://CDS.VizieR/J/ApJ/764/78</identifier><altIdentifier>doi:10.26093/cds/vizier.17640078</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ramirez I.</name></creator><creator><name>Allende Prieto C.</name></creator><creator><name>Lambert D.L.</name></creator><date role="Updated">2017-07-04T07:09:23Z</date><date role="Created">2014-04-29T07:56:50Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>chemical-abundances</subject><subject>radial-velocity</subject><subject>g-stars</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>line-intensities</subject><description>Atmospheric parameters and oxygen abundances of 825 nearby FGK stars are derived using high-quality spectra and a non-local thermodynamic equilibrium analysis of the 777nm OI triplet lines. We assign a kinematic probability for the stars to be thin-disk (P_1_), thick-disk (P_2_), and halo (P_3_) members. We confirm previous findings of enhanced [O/Fe] in thick-disk (P_2_&gt;0.5) relative to thin-disk (P_1_&gt;0.5) stars with [Fe/H]&lt;~-0.2, as well as a "knee" that connects the mean [O/Fe]-[Fe/H] trend of thick-disk stars with that of thin-disk members at [Fe/H]&gt;~-0.2. Nevertheless, we find that the kinematic membership criterion fails at separating perfectly the stars in the [O/Fe]-[Fe/H] plane, even when a very restrictive kinematic separation is employed. Stars with "intermediate" kinematics (P_1_&lt;0.7, P_2_&lt;0.7) do not all populate the region of the [O/Fe]-[Fe/H] plane intermediate between the mean thin-disk and thick-disk trends, but their distribution is not necessarily bimodal. Halo stars (P_3_&gt;0.5) show a large star-to-star scatter in [O/Fe]-[Fe/H], but most of it is due to stars with Galactocentric rotational velocity V&lt;-200km/s; halo stars with V&gt;-200km/s follow an [O/Fe]-[Fe/H] relation with almost no star-to-star scatter. Early mergers with satellite galaxies explain most of our observations, but the significant fraction of disk stars with "ambiguous" kinematics and abundances suggests that scattering by molecular clouds and radial migration have both played an important role in determining the kinematic and chemical properties of solar neighborhood stars.</description><source format="bibcode">2013ApJ...764...78R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/764/78</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/pastel">B/pastel : The PASTEL catalogue (Soubiran+, 2010-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/190">III/190 : WEB Catalog of Radial Velocities (Duflot+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/238">I/238 : Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/89">V/89 : Ages, Metallicities, Galactic Orbit of F stars (Marsakov+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/184">III/184 : 3rd Bibliog. 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J/A+A/465/271</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Teff</name><description>[4215/6989] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[22/129] Uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[1.2/4.8] Log of the surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logg</name><description>[0/0.3] Uncertainty in logg</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-2.8/0.4] Metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]</name><description>[0.02/0.3] Uncertainty in [Fe/H]</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vt</name><description>[0/2.5] Turbulent velocity</description><unit>km/s</unit><ucd>phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_Vt</name><description>[+] Vt adopted (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[Fe/H]1</name><description>Metallicity derived from FeI lines</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]1</name><description>Uncertainty in [Fe/H]1</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]2</name><description>Metallicity derived from FeII lines</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]2</name><description>Uncertainty in [Fe/H]2</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sample</name><description>Sample name (giant, main, manual or noplx) (5)</description><ucd>meta.id;src.sample</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Age</name><description>[0.4/14.7]? Stellar age</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e1Age</name><description>Lower 1{sigma} uncertainty in Age</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E1Age</name><description>Upper 1{sigma} uncertainty in Age</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e2Age</name><description>Lower 2{sigma} uncertainty in Age</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E2Age</name><description>Upper 2{sigma} uncertainty in Age</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M</name><description>[0.6/2.2]? Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e1M</name><description>Lower 1{sigma} uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E1M</name><description>Upper 1{sigma} uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e2M</name><description>Lower 2{sigma} uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E2M</name><description>Upper 2{sigma} uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L7772</name><description>[0/9.6] LTE derived [O/H] abundance from 7772{AA} line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L7774</name><description>LTE derived [O/H] abundance from 7774{AA} line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L7775</name><description>LTE derived [O/H] abundance from 7775{AA} line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N7772</name><description>NLTE derived [O/H] abundance from 7772{AA} line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N7774</name><description>NLTE derived [O/H] abundance from 7774{AA} line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N7775</name><description>NLTE derived [O/H] abundance from 7775{AA} line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[O/H]L</name><description>[-1.6/0.7] Differential LTE derived [O/H] abundance</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[O/H]L</name><description>Uncertainty in [O/H]LTE</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[O/H]N</name><description>[-3.9/0.6] Differential NLTE derived [O/H] abundance</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[O/H]N</name><description>Uncertainty in [O/H]NLTE</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Positions from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/764/78/table3</name><description>Iron Line List</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambda</name><description>[4576.3/7711.8] Wavelength; in Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ID</name><description>Fe species identifier</description><ucd>meta.id;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>ExPot</name><description>[0.08/5] Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(gf)</name><description>[-5/-0.2] Log of oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EW</name><description>[9/123] Equivalent width (in m{AA})</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>