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<ri:Resource created="2018-07-26T09:34:36Z" status="active" updated="2025-05-19T09:50:00Z" 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>Binaries with F, G or K primaries and M dwarfs</title><shortName>J/MNRAS/479/1332</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/479/1332</identifier><altIdentifier>doi:10.26093/cds/vizier.74791332</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Montes D.</name></creator><creator><name>Gonzalez-Peinado R.</name></creator><creator><name>Tabernero H.M.</name></creator><creator><name>Caballero J.A.</name></creator><creator><name>Marfil E.,Alonso-Floriano F.J.</name></creator><creator><name>Cortes-Contreras M.</name></creator><creator><name>Gonzalez Hernandez J.I.,Klutsch A.</name></creator><creator><name>Moreno-Jodar C.</name></creator><date role="Updated">2024-08-18T20:20:31Z</date><date role="Created">2018-07-26T09:34:36Z</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>multiple-stars</subject><subject>m-stars</subject><subject>dwarf-stars</subject><description>We investigated almost 500 stars distributed among 193 binary or multiple systems made of late-F, G-, or early-K primaries and late-K or M dwarf companion candidates. For all of them, we compiled or measured coordinates, J-band magnitudes, spectral types, distances, and proper motions. With these data, we established a sample of 192 physically bound systems. In parallel, we carried out observations with HERMES/Mercator and obtained high-resolution spectra for the 192 primaries and five secondaries. We used these spectra and the automatic STEPAR code for deriving precise stellar atmospheric parameters: Teff, logg, {xi}, and chemical abundances for 13 atomic species, including [Fe/H]. After computing Galactocentric space velocities for all the primary stars, we performed a kinematic analysis and classified them in different Galactic populations and stellar kinematic groups of very different ages, which match our own metallicity determinations and isochronal age estimations. In particular, we identified three systems in the halo and 33 systems in the young Local Association, Ursa Major and Castor moving groups, and IC 2391 and Hyades Superclusters. We finally studied the exoplanet-metallicity relation in our 193 primaries and made a list 13 M-dwarf companions with very high metallicity that can be the targets of new dedicated exoplanet surveys. 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Microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_xi</name><description>? rms uncertainty on xi</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>? Metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Fe/H]</name><description>? rms uncertainty on [Fe/H]</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]lit</name><description>? 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[Ti/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Ti/H]</name><description>? rms uncertainty on [Ti/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[V/H]</name><description>? [V/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[V/H]</name><description>? rms uncertainty on [V/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Cr/H]</name><description>? [Cr/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Cr/H]</name><description>? rms uncertainty on [Cr/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Mn/H]</name><description>? [Mn/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Mn/H]</name><description>? rms uncertainty on [Mn/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Co/H]</name><description>? [Co/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Co/H]</name><description>? rms uncertainty on [Co/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ni/H]</name><description>? [Ni/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Ni/H]</name><description>? rms uncertainty on [Ni/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/479/1332/tableb5</name><description>Kinematics of late-F-, G-, and late-K stars</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>WDS</name><description>WDS designation (HHMMm+DDMM)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Name</name><description>Name</description><ucd>meta.id</ucd></column><column><name>n_Name</name><description>[a] Note on Name (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RV</name><description>Radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RV</name><description>? rms uncertainty on RV</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Uvel</name><description>U velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Uvel</name><description>rms uncertainty on Uvel</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vvel</name><description>V velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vvel</name><description>rms uncertainty on Vvel</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Wvel</name><description>W velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Wvel</name><description>rms uncertainty on Wvel</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pop</name><description>Population (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>SKG</name><description>Stellar Kinematic Group (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>SKGl</name><description>Stellar Kinematic Group from literature</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>rSKGl</name><description>Reference for SKGl (4)</description><ucd>meta.bib</ucd></column></table><table><name>J/MNRAS/479/1332/refs</name><description>References</description><column><name>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><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>Ref</name><description>Reference code</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>BibCode</name><description>BibCode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Aut</name><description>Author's name</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column></table></schema></tableset></ri:Resource>