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<ri:Resource created="2006-10-01T17:16:06Z" 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>Grid of close binaries experiencing mass exchange</title><shortName>J/A+A/455/247</shortName><identifier>ivo://CDS.VizieR/J/A+A/455/247</identifier><altIdentifier>doi:10.26093/cds/vizier.34550247</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tian B.</name></creator><creator><name>Deng L.</name></creator><creator><name>Han Z.</name></creator><creator><name>Zhang X.B.</name></creator><date role="Updated">2006-10-01T17:19:08Z</date><date role="Created">2006-10-01T17:16:06Z</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>eclipsing-binary-stars</subject><subject>stellar-evolutionary-models</subject><subject>stellar-masses</subject><description>To simulate the population of the primordial blue stragglers in old open clusters, a grid of close binaries experiencing mass exchange is needed. To this aim, various combinations that can trigger mass exchange for the donor masses of 0.1M_{sun}_ to 2.0M_{sun}_ are calculated with a fine grid in parameters. The mass range of the accretor is from 0.1M_{sun}_ to the mass of the corresponding donor. The mass intervals of the donors and the accretors are all 0.1M_{sun}_. To cover all possible cases of close binaries, the orbit separation ranges from 1.0 to 50.0R_{sun}_ with a grid interval of 1.0R_{sun}_. Following the numerical scheme described above, a grid for six ages from 1.0Gyr to 6.0Gyr is obtained. In this table, mass, effective temperature, luminosity, gravity, Hydrogen abundance in the core, Helium abundance in the core, B magnitude, V magnitude, B-V color, mass ratio, orbital separation and period of the close binaries experiencing mass exchange are given.</description><source format="bibcode">2006A&amp;A...455..247T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/455/247</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/J/A+AS/131/395">J/A+AS/131/395 : Eclipsing binaries light curves models (Claret 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/79/259">J/AZh/79/259 : Intermediate-Mass Eclipsing Binaries Models (Kovaleva, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/79/738">J/AZh/79/738 : Binary stars population model in the Galaxy (Tutukov+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/490/328">J/ApJ/490/328 : "Mass Discrepancy" for Massive Stars (Burkholder+ 1997)</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/455/247</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/455/247</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/455/247</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/455/247</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/455/247</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/455/247</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/455/247/table2</name><description>A grid of close binaries experiencing mass exchange</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>M1i</name><description>The initial mass of the accretor</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>M2i</name><description>The initial mass of the donor</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>qi</name><description>The initial mass ratio of the binary</description><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ai</name><description>The initial separation of the binary</description><unit>solRad</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Peri</name><description>The initial period of the binary</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Age</name><description>The age of the binary</description><unit>1e+09yr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M1</name><description>The mass of the accretor</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logTeff1</name><description>The effective temperature of the accretor</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL1</name><description>The luminosity of the accretor</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>log(g1)</name><description>The gravity of the accretor</description><unit>log(m.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>H1</name><description>The Hydrogen abundance in the core of the accretor</description><ucd>phys.abund.X</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>He1</name><description>The Helium abundance in the core of the accretor</description><ucd>phys.abund.Y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag1</name><description>B magnitude of the accretor</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Vmag1</name><description>V magnitude of the accretor</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>(B-V)1</name><description>B-V color index of the accretor</description><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>M2</name><description>The mass of the donor</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logTeff2</name><description>The effective temperature of the donor</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL2</name><description>The luminosity of the donor</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>log(g2)</name><description>The gravity of the donor</description><unit>log(m.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>H2</name><description>The Hydrogen abundance in the core of the donor</description><ucd>phys.abund.X</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>He2</name><description>The Helium abundance in the core of the donor</description><ucd>phys.abund.Y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag2</name><description>B magnitude of the donor</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Vmag2</name><description>V magnitude of the donor</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>(B-V)2</name><description>B-V color index of the donor</description><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>q</name><description>The mass ratio of the binary</description><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>A</name><description>The separation of the binary</description><unit>solRad</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>The period of the binary</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Bmag</name><description>B magnitude of the binary</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Vmag</name><description>V magnitude of the binary</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B-V</name><description>B-V color index of the binary</description><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType 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