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<ri:Resource created="2020-09-30T07:39:58Z" 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>Parameters &amp; abundances for Hyades/Field G-K dwarfs</title><shortName>J/AJ/159/174</shortName><identifier>ivo://CDS.VizieR/J/AJ/159/174</identifier><altIdentifier>doi:10.26093/cds/vizier.51590174</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Takeda Y.</name></creator><creator><name>Honda S.</name></creator><date role="Updated">2021-09-13T14:56:49Z</date><date role="Created">2020-09-30T07:39:58Z</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>dwarf-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>effective-temperature</subject><subject>chemical-abundances</subject><description>It has been suggested that Fe abundances of K dwarfs derived from FeI and FeII lines show considerable discrepancies, and oxygen abundances determined from high-excitation OI-7771-5 triplet lines are appreciably overestimated (the problem becoming more serious toward lower Teff), which, however, has not yet been widely confirmed. With the aim of clarifying this issue, we spectroscopically determined the atmospheric parameters of 148 G-K dwarfs (Hyades cluster stars and field stars) by assuming the classical FeI/FeII ionization equilibrium as usual, and determined their oxygen abundances by applying the non-local thermal equilibrium spectrum fitting analysis to OI-7771-5 lines. It turned out that the resulting parameters did not show any significant inconsistency with those determined by other methods (for example, the mean differences in Teff and logg from the well-determined solutions of Hyades dwarfs are mostly &lt;~100K and &lt;~0.1dex). Likewise, the oxygen abundances of Hyades stars are around [O/H]~+0.2dex (consistent with the metallicity of this cluster) without exhibiting any systematic Teff-dependence. Accordingly, we conclude that parameters can be spectroscopically evaluated to a sufficient precision in the conventional manner (based on the Saha-Boltzmann equation for FeI/FeII) and oxygen abundances can be reliably determined from the OI-7771-5 triplet for K dwarfs as far as stars of Teff&gt;~4500K are concerned. We suspect that previously reported strongly Teff-dependent discrepancies may have stemmed mainly from overestimation of weak-line strengths and/or improper Teff scale.</description><source format="bibcode">2020AJ....159..174T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/159/174</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/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/367/111">J/A+A/367/111 : A Hipparcos study of the Hyades cluster (de Bruijne+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/394/927">J/A+A/394/927 : Age-metallicity relation for nearby stars (Ibukiyama+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/336/879">J/MNRAS/336/879 : G and K dwarfs UBV(RI)c and ubvy photometry (Kotoneva+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/402/343">J/A+A/402/343 : IR O I triplet, [OI] lines in F-K dwarfs/giants (Takeda,2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/420/183">J/A+A/420/183 : Spectro. survey in solar neighborhood (Allende Prieto+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/602/L117">J/ApJ/602/L117 : Oxygen in Pleiades and M34 dwarfs (Schuler+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/57/65">J/PASJ/57/65 : CNO abundances of solar-type stars (Takeda+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/57/27">J/PASJ/57/27 : Atmospheric parameters of nearby F-K stars (Takeda+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/59/335">J/PASJ/59/335 : Properties of 160 F-K disk dwarfs/subgiants (Takeda+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A54">J/A+A/512/A54 : Teff and Fbol from Infrared Flux Method (Casagrande+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/735/41">J/ApJ/735/41 : Carbon and oxygen abundances in FGK stars (Petigura+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/415/563">J/MNRAS/415/563 : Elemental abundances in Hyades supercluster (De Silva+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/164">J/ApJ/757/164 : Oxygen abundances of dwarf stars (Ramirez+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/78">J/ApJ/764/78 : Oxygen abundances in nearby FGK stars (Ramirez+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/594/A43">J/A+A/594/A43 : APOGEE/Kepler sample stars abundances (Hawkins+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/21">J/AJ/153/21 : Abund. in local region.II. 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