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<ri:Resource created="2009-07-04T18:19:42Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>PMS tracks at low Z for 0.1&lt;=M&lt;=1.5</title><shortName>J/A+A/496/223</shortName><identifier>ivo://CDS.VizieR/J/A+A/496/223</identifier><altIdentifier>doi:10.26093/cds/vizier.34960223</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Di Criscienzo M.</name></creator><creator><name>Ventura P.</name></creator><creator><name>D'antona F.</name></creator><date role="Updated">2017-06-30T05:48:44Z</date><date role="Created">2009-07-04T18:19:42Z</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>pre-main-sequence-stars</subject><subject>stellar-evolutionary-models</subject><description>While MLT-alpha^2D^ models are not available for lower metallicities, we extend to lower Z the NEMO-FST models, under the hypothesis that in such a way we are simulating the results of MLT-alpha^2D^ models also at smaller Z. We use standard stellar computation techniques in which the atmospheric boundary conditions are derived making use of model atmosphere grids. This allows us to take into account the non greyness of the atmosphere, but adds a new parameter to the stellar structure uncertainty, namely the efficiency of convection in the atmospheric structure, if convection is computed in the atmospheric grid by a model different to the model adopted for the interior integration.</description><source format="bibcode">2009A&amp;A...496..223D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/496/223</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VI/109">VI/109 : Population Synthesis Models at very low Z (Schaerer, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/113">VI/113 : Evolutionary models of Population II stars (Cariulo+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/361/1023">J/A+A/361/1023 : Evolution models for {alpha}-enhanced stars (Salasnich+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/141/371">J/A+AS/141/371 : Low-mass stars evolutionary tracks+isochrones (Girardi+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/484/815">J/A+A/484/815 : Scaled solar tracks and isochrones (Bertelli+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/494/209">J/A+A/494/209 : Pre-main sequence evolutionary tracks (Landin+, 2009)</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/A+A/496/223</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/496/223</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/496/223</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/496/223</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/496/223</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/496/223</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/496/223/tracks</name><description>Evolutionary tracks</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>Code</name><description>[AH97 NEMO] Code used (1)</description><ucd>meta.id;stat.fit</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Z</name><description>Initial metallicity (0.0002, 0.002 or 0.006)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>Initial mass (from 0.1 to 1.5)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Age)</name><description>Stellar age</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL</name><description>Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Teff)</name><description>Effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/496/223/iso</name><description>Isochrones</description><column><name>logL</name><description>Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</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>Z</name><description>Isochone metallicity (0.0002, 0.002 or 0.006)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age</name><description>Isochone age (1e+5, 1e+6 or 1e+7)</description><unit>yr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>Mass (from 0.1 to 1.5)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Teff)</name><description>Effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>