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<ri:Resource created="2023-02-10T13:20:26Z" 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>Masses and radii of Kepler and CoRoT targets</title><shortName>J/MNRAS/489/1753</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/489/1753</identifier><altIdentifier>doi:10.26093/cds/vizier.74891753</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yildiz M.</name></creator><creator><name>Celik Orhan Z.</name></creator><creator><name>Kayhan C.</name></creator><date role="Updated">2024-08-20T20:12:39Z</date><date role="Created">2023-02-10T13:20:26Z</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>late-type-stars</subject><subject>asteroseismology</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><subject>stellar-radii</subject><subject>stellar-distance</subject><subject>visible-astronomy</subject><description>Recently, by analysing the oscillation frequencies of 90 stars, Yildiz, Celik Orhan &amp; Kayhan have shown that the reference frequencies ({nu}_min0_, {nu}_min1_, and {nu}_min2_) derived from glitches due to He II ionization zone have very strong diagnostic potential for the determination of their effective temperatures. In this study, we continue to analyse the same stars and compute their mass, radius, and age from different scaling relations including relations based on {nu}_min0_, {nu}_min1_, and {nu}_min2_. For most of the stars, the masses computed using {nu}_min0_ and {nu}_min1_ are very close to each other. For 38 stars, the difference between these masses is less than 0.024 M_{sun}_. The radii of these stars from {nu}_min0_ and {nu}_min1_ are even closer, with differences of less than 0.007R_{sun}_. These stars may be the most well known solar-like oscillating stars and deserve to be studied in detail. The asteroseismic expressions we derive for mass and radius show slight dependence on metallicity. We therefore develop a new method for computing initial metallicity from this surface metallicity by taking into account the effect of microscopic diffusion. The time dependence of initial metallicity shows some very interesting features that may be important for our understanding of chemical enrichment of Galactic Disc. According to our findings, every epoch of the disc has its own lowest and highest values for metallicity. It seems that rotational velocity is inversely proportional to 1/2 power of age as given by the Skumanich relation.</description><source format="bibcode">2019MNRAS.489.1753Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/489/1753</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/corot">B/corot : CoRoT observation log (N2-4.4) (CoRoT 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration 2018)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/489/1753</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/489/1753</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/489/1753</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/489/1753</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/489/1753</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/489/1753</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/489/1753/tableb1 (Basic properties of Kepler and CoRoT targets)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/489/1753/tableb1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/489/1753/tableb1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/489/1753/tableb1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>292.0826839</ra><dec>37.0598342</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/14578 14581 14585 14751 14763 14767 14770-14771 14777-14779 14794 14819 14824 14827 14918 14921-14922 14924-14926 14930-14932 14935-14936 14938-14939 14941 14947-14948 14956 14959-14960 14963 14967 14969 14973 15041 15044 15057 15061-15062 15106 15109-15110 15112 15121 15124 15129 15131-15133 15142 15145-15146 15154-15157 15168-15170 15172-15174 15178 22036 22120 22122 22300 23575 30289 30294 30878 33281 45485</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/489/1753?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/489/1753/tableb1</name><description>Basic properties of Kepler and CoRoT targets</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType><flag>nullable</flag></column><column><name>e_TeS</name><description>Error on TeS</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Error on numin1</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>numin2</name><description>? Reference frequency for min2</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_numin2</name><description>? Error on numin2</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dnu</name><description>Mean large separation between oscillation frequencies</description><unit>uHz</unit><ucd>pos.angDistance;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Dnu</name><description>Error on Dnu</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dnu</name><description>? Mean small separation between oscillation frequencies</description><unit>uHz</unit><ucd>pos.angDistance;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>TeS</name><description>Effective temperature from spectra (see Section 2 in Paper III) (2)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>TeVK</name><description>? Effective temperature from V-K colour (see Section 2 in Paper III) (2)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_TeVK</name><description>? Error on TeVK</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>TeBV</name><description>? Effective temperature from B-V colour (see Section 2 in Paper III) (2)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_TeBV</name><description>? Error on TeBV</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Tsis0</name><description>? Effective temperature from min0 (see Section 2 in Paper III) (2)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Tsis0</name><description>? Error on Tsis0</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Tsis1</name><description>? Effective temperature from min1 (see Section 3 in Paper III) (2)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Tsis1</name><description>? Error on Tsis1</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Tsis2</name><description>? Effective temperature from min2 (see Section 3 in Paper III) (2)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Tsis2</name><description>? 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Error on Mlit</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rsca</name><description>Star radius from new scaling relation (see Section 3 in Paper III) (2)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rsca</name><description>Error on Rsca</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rsis0</name><description>? Star radius from min0 (see Section 3 in Paper III) (2)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Rsis0</name><description>? Error on Rsis0</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rsis1</name><description>? Star radius from min1 (see Section 3 in Paper III) (2)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Rsis1</name><description>? Error on Rsis1</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rlit</name><description>? Star radius from litterature</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Rlit</name><description>? Error on Rlit</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dobs</name><description>? Distance from litterature</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_dobs</name><description>? Error on dobs</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dsis</name><description>? Distance from seismic</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_dsis</name><description>? 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