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<ri:Resource created="2026-04-20T08:48:50Z" status="active" updated="2026-04-20T07:49:14Z" 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>9Msun ultramassive WD stars progenitor</title><shortName>J/MNRAS/548/G469</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/548/G469</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Antonini A.S.R.</name></creator><creator><name>Romero A.D.</name></creator><creator><name>Kepler S.O.</name></creator><date role="Updated">2026-04-20T07:49:14Z</date><date role="Created">2026-04-20T08:48:50Z</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>galaxies</subject><subject>stellar-spectral-types</subject><subject>early-type-stars</subject><subject>late-type-stars</subject><subject>supergiant-stars</subject><subject>white-dwarf-stars</subject><subject>astronomical-models</subject><description>We study the full evolution of a 1.313M_{sun}_ white dwarf star that descended from a 9M_{sun}_ main-sequence progenitor with an initial metallicity of Z=0.02. Using MESA r24.08.01, we calculate its entire evolution from pre-ZAMS to the WD cooling curve, including both the evolution through 139 thermal pulses and the post-AGB phase. The resulting remnant is an ultramassive H-deficient WD, for which the composition, in mass fraction, is 47.7% ^16^O, 39.7% ^20^Ne, 4.2% ^24^Mg, 3.3% ^23^Na and 0.386% ^12^C -- corresponding to a total mass of 5x10^-3^M_{sun}_ of C --, surrounded by a 1.5x10^-5^M_{sun}_ He layer. We also investigate the effects of fully suppressing the TP-SAGB stage by adopting a high mass-loss rate only after the second dredge-up, and find only minor differences in the final mass and composition. In addition, we calculate models with and without phase separation during the WD stage, estimating a cooling delay of only 16Myr. This is the first ultramassive white dwarf sequence for which both the TP-SAGB and post-AGB stages are calculated and, to our knowledge, the most massive WD model from complete evolution for which cooling times and detailed abundance profiles are published.</description><source format="bibcode">2026MNRAS.548ag469A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/548/G469</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/548/G469</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/548/G469</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/548/G469</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/548/G469</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/548/G469</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/548/G469</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/MNRAS/548/G469/baseline</name><description>cooling data for our baseline model</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>logTeff</name><description>Effective temperature in log scale</description><unit>log(K)</unit><ucd>phys.temperature.effective;instr.scale</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logL</name><description>Luminosity in log scale</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logg</name><description>Surface gravity in log scale</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logR</name><description>Radius in log scale</description><unit>log(solRad)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>tcool</name><description>Cooling age</description><unit>yr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logPc</name><description>Central Pressure in log scale</description><unit>log(1e-07J.cm**-3)</unit><ucd>phys.pressure</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logrhoc</name><description>Central density in log scale</description><unit>log(g.cm**-3)</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTc</name><description>Central Temperature in log scale</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Gammac</name><description>Central coulomb interaction parameter</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/548/G469/nops</name><description>cooling data for our model calculated without phase separation (noPS)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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