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<ri:Resource created="2004-10-03T16:34:43Z" 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>Evolutionary models of Population II stars</title><shortName>VI/113</shortName><identifier>ivo://CDS.VizieR/VI/113</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cariulo P.</name></creator><creator><name>Castellani V.</name></creator><creator><name>Degl'Innocenti S.</name></creator><date role="Updated">2017-07-12T13:41:06Z</date><date role="Created">2004-10-03T16:34:43Z</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>stellar-evolutionary-models</subject><subject>population-ii-stars</subject><description>The models are calculated for different chemical compositions both without overshooting (standard models, including microscopic diffusion of He and heavy elements) and with different overshooting efficiency. Each set of models can be found in a different sub-directory. It is possible to get all the content for each chemical composition, the content of each selected sub-directory or just a given file. In each directory there are evolutionary tracks (TRACKS), isochrones (ISOCHRONES), horizontal branch models together with a table of the ZAHB characteristics (HB) and files with some relevant physical values of selected models (STRUCTURES). Models with overshooting are calculated for masses higher than 1M_{sun}_ to avoid the unobserved presence of the overall contraction feature in 1M_{sun}_ stars. Thus isochrones for ages higher than about 5Gyr are the same as in the standard case and thus are not included in the overshooting directories. Models with overshooting does not include microscopic diffusion because for masses higher than about 1M_{sun}_ the effect of this mechanism is almost negligible. Models with overshooting are calculated for masses higher than 1M_{sun}_ to avoid the unobserved presence of the overall contraction feature in 1M_{sun}_ stars. Thus isochrones for ages higher than about 5Gyr are the same as in the standard case and thus are not included in the overshooting directories. Models with overshooting does not include microscopic diffusion because for masses higher than about 1M_{sun}_ the effect of this mechanism is almost negligible. All the tracks and isochrones have been transformed in the observation plane by adopting the model atmospheres by Castelli (1999A&amp;A...346..564C), see also Castelli, Gratton &amp; Kurucz (1997A&amp;A...318..841C). For convenience, all tracks and isochrones have been grouped in 4 tables tracks.dat, struct.dat, hb.dat and isochron.dat</description><source format="bibcode">2004A&amp;A...421.1121C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/VI/113</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>http://astro.df.unipi.it/SAA/PEL/Z0.html : Pisa Evolutionary Library</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/96">VI/96 : Evolutionary Sequences (Fagotto+ 1993-96)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/96/269">J/A+AS/96/269 : Grids of stellar models I (Schaller+, 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/98/523">J/A+AS/98/523 : Grids of stellar models II (Schaerer+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/101/415">J/A+AS/101/415 : Grids of stellar models III (Charbonnel+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/102/339">J/A+AS/102/339 : Grids of stellar models IV (Schaerer+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/103/97">J/A+AS/103/97 : Grids of stellar models V (Meynet+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/115/339">J/A+AS/115/339 : Grids of stellar models VI (Charbonnel+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/128/471">J/A+AS/128/471 : Grids of stellar models VII (Mowlavi+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/135/405">J/A+AS/135/405 : Grids of stellar models VIII (Charbonnel+ 1999)</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=VI/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=VI/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=VI/113</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=VI/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=VI/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=VI/113</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>VI/113/hb</name><description>*Evolutionary tracks in Horizontal Branch stage</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Ratio overshooting length / pressure height (in models with overshooting)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PHS</name><description>[PH] Pre-main-sequence/Horizontal-branch stage.</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logt</name><description>? Age (does not always exist)</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Mass</name><description>Mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logL</name><description>Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTe</name><description>Effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>VMAG</name><description>Absolute V magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B-V</name><description>B-V colour index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>U-B</name><description>U-B colour index</description><unit>mag</unit><ucd>phot.color;em.opt.U;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>V-I</name><description>V-I colour index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>V-R</name><description>V-R colour index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R-I</name><description>R-I colour index</description><unit>mag</unit><ucd>phot.color;em.opt.R;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>VI/113/strfiles</name><description>List of files with structure parameters</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>File</name><description>Name of model file, in "models" subdirectory</description><ucd>meta.id;stat.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType" arraysize="44*">char</dataType></column><column><name>Z</name><description>Initial metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Initial He abundance</description><ucd>phys.abund.Y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha</name><description>Ratio mixing length / pressure scale height</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mo</name><description>Initial mass (mass of progenitor)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diff</name><description>[d] Model with diffusion</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>beta</name><description>? Ratio overshooting length / pressure height (in models with overshooting)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Plot</name><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>VI/113/trkfiles</name><description>List of files with evolutionary tracks</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Ratio overshooting length / pressure height (in models with overshooting)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logL</name><description>Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTe</name><description>Effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>VMAG</name><description>Absolute V magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B-V</name><description>B-V colour index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>U-B</name><description>U-B colour index</description><unit>mag</unit><ucd>phot.color;em.opt.U;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>V-I</name><description>V-I colour index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>V-R</name><description>V-R colour index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R-I</name><description>R-I colour index</description><unit>mag</unit><ucd>phot.color;em.opt.R;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>VI/113/hbfiles</name><description>List of files with evolutionary tracks in Horizontal Branch (He-burning)</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>File</name><description>Name of model file, in "models" subdirectory</description><ucd>meta.id;stat.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType" arraysize="44*">char</dataType></column><column><name>Z</name><description>Initial metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Initial He abundance</description><ucd>phys.abund.Y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha</name><description>Ratio mixing length / pressure scale height</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mo</name><description>Initial mass (mass of progenitor)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diff</name><description>[d] Model with diffusion</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Mass</name><description>? 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Ratio overshooting length / pressure height (in models with overshooting)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logt</name><description>Age</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>H/He</name><description>Central abundance of H/He</description><ucd>phys.abund</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">double</dataType></column><column><name>logTe</name><description>Effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTc</name><description>Central temperature</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logrhoc</name><description>Central density</description><unit>log(g.cm**-3)</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTmax</name><description>Central maximum temperature</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MassTm</name><description>Mass coordinate of the maximum in temperature (M/Mtot)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MassCC</name><description>Mass extension of the central convective region</description><unit>solMass</unit><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MassHeC</name><description>Mass extension of the helium core</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MassCE</name><description>Mass coordinate of the bottom of the convective envelope (M/Mtot)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L-pp</name><description>Fraction of the luminosity of the proton-proton chain over the total luminosity</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L-CNO</name><description>Fraction of the luminosity of the CNO cycle over the total luminosity</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L-He</name><description>Fraction of the luminosity of the He burning over the total luminosity</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>L-Gra</name><description>Fraction of the luminosity of the gravothermal energy over the total luminosity</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>VI/113/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>Z</name><description>Initial metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Initial He abundance</description><ucd>phys.abund.Y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha</name><description>Ratio mixing length / local pressure scale height</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mo</name><description>Initial mass (mass of progenitor)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diff</name><description>[d] Model with diffusion</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>beta</name><description>? Ratio overshooting length / pressure height (in models with overshooting)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PHS</name><description>[PH] Pre-main-sequence/Horizontal-branch stage.</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logt</name><description>? Age (does not always exist)</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Mass</name><description>Mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logL</name><description>Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTe</name><description>Effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>VMAG</name><description>Absolute V magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B-V</name><description>B-V colour index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>U-B</name><description>U-B colour index</description><unit>mag</unit><ucd>phot.color;em.opt.U;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>V-I</name><description>V-I colour index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>V-R</name><description>V-R colour index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R-I</name><description>R-I colour index</description><unit>mag</unit><ucd>phot.color;em.opt.R;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>