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<ri:Resource created="2018-09-25T09:44:00Z" 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>Full Evolutionary Sequences of Massive WDs</title><shortName>J/MNRAS/480/1547</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/480/1547</identifier><altIdentifier>doi:10.26093/cds/vizier.74801547</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lauffer G.R.</name></creator><creator><name>Romero A.D.</name></creator><creator><name>Kepler S.O.</name></creator><date role="Updated">2024-08-18T20:21:02Z</date><date role="Created">2018-09-25T09:44:00Z</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>astronomical-models</subject><subject>stellar-atmospheres</subject><subject>white-dwarf-stars</subject><description>We explore the evolution of hydrogen-rich and hydrogen-deficient white dwarf stars with masses between 1.012 and 1.307M_{sun}, and initial metallicity of Z=0.02. These sequences are the result of main-sequence stars with masses between 8.8 and 11.8M_{sun}. The simulations were performed with MESA (Modules for Experiments in Stellar Astrophysics), starting at the zero-age main sequence, through thermally pulsing and mass-loss phases, ending at the white dwarf cooling sequence. We present reliable chemical profiles for the whole mass range considered, covering the different expected central compositions (i.e. C/O, O/Ne and Ne/O/Mg) and its dependence on the stellar mass. In addition, we present detailed chemical profiles of hybrid C/O-O/Ne core white dwarfs, found in the mass range between 1.024 and 1.15M_{sun}. We present the initial-to-final mass relation, the mass-radius relation and cooling times considering the effects of atmosphere and core composition.</description><source format="bibcode">2018MNRAS.480.1547L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/480/1547</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/480/1547</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/480/1547</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/480/1547</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/480/1547</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/480/1547</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/480/1547</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/480/1547/table1</name><description>List of evolutionary tracks sequences</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>MZAMS</name><description>Values of initial mass at ZAMS</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MWD</name><description>White dwarfs mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>mlogMH/MWD</name><description>Hydrogen content for H-rich sequence (-logMH/MWD)</description><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>mlogMHe/MWD</name><description>Helium content for H-rich sequence (-logMHe/MWD)</description><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NameH</name><description>Name of evolutionary tracks sequence with H atmosphere in subdirectory tracks</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>NameHe</name><description>Name of evolutionary tracks sequence with He atmosphere in subdirectory tracks</description><ucd>meta.id;time.age;obs.atmos</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column></table></schema></tableset></ri:Resource>