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<ri:Resource created="2022-02-18T13:14:23Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>Model atmosphere analysis of hot WDs from SDSS DR12</title><shortName>J/ApJ/901/93</shortName><identifier>ivo://CDS.VizieR/J/ApJ/901/93</identifier><altIdentifier>doi:10.26093/cds/vizier.19010093</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bedard A.</name></creator><creator><name>Bergeron P.</name></creator><creator><name>Brassard P.</name></creator><creator><name>Fontaine G.</name></creator><date role="Updated">2023-06-05T09:52:14Z</date><date role="Created">2022-02-18T13:14:23Z</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>white-dwarf-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>stellar-spectral-types</subject><subject>stellar-masses</subject><subject>stellar-radii</subject><subject>effective-temperature</subject><description>As they evolve, white dwarfs undergo major changes in surface composition, a phenomenon known as spectral evolution. In particular, some stars enter the cooling sequence with helium atmospheres (type DO) but eventually develop hydrogen atmospheres (type DA), most likely through the upward diffusion of residual hydrogen. Our empirical knowledge of this process remains scarce: the fractions of white dwarfs that are born helium rich and that experience the DO-to-DA transformation are poorly constrained. We tackle this issue by performing a detailed model-atmosphere investigation of 1806 hot (Teff&gt;=30000K) white dwarfs observed spectroscopically by the Sloan Digital Sky Survey. We first introduce our new generations of model atmospheres and theoretical cooling tracks, both appropriate for hot white dwarfs. We then present our spectroscopic analysis, from which we determine the atmospheric and stellar parameters of our sample objects. We find that ~24% of white dwarfs begin their degenerate life as DO stars, among which ~2/3 later become DA stars. We also infer that the DO-to-DA transition occurs at substantially different temperatures (75000K&gt;Teff&gt;30000K) for different objects, implying a broad range of hydrogen content within the DO population. Furthermore, we identify 127 hybrid white dwarfs, including 31 showing evidence of chemical stratification, and we discuss how these stars fit in our understanding of the spectral evolution. Finally, we uncover significant problems in the spectroscopic mass scale of very hot (Teff&gt;60000K) white dwarfs.</description><source format="bibcode">2020ApJ...901...93B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/901/93</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/207">II/207 : Palomar-Green catalog UV-excess stellar objects (Green+ 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/133/413">J/ApJS/133/413 : BVRIJHK photometry of cool white dwarfs (Bergeron+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/156/47">J/ApJS/156/47 : DA WDs from the Palomar Green Survey (Liebert+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/167/40">J/ApJS/167/40 : SDSS4 confirmed white dwarfs catalog (Eisenstein+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/676">J/AJ/132/676 : SDSS hot DB white dwarfs (Eisenstein+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/652/1554">J/ApJ/652/1554 : Iron in hot DA white dwarfs (Vennes+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/138">J/ApJ/743/138 : Spectroscopic survey of bright WDs (Gianninas+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/730/128">J/ApJ/730/128 : Spectroscopy of DA WD from the SDSS-DR4 (Tremblay+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/204/5">J/ApJS/204/5 : SDSS DR7 white dwarf catalog (Kleinman+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/555/A96">J/A+A/555/A96 : White dwarf cooling timescales (Salaris+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/583/A86">J/A+A/583/A86 : DB white dwarfs in SDSS DR10 and DR12 (Koester+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/446/4078">J/MNRAS/446/4078 : New white dwarf stars in SDSS DR10 (Kepler+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/455/3413">J/MNRAS/455/3413 : New WD and subdwarf stars in SDSS DR12 (Kepler+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/848/11">J/ApJ/848/11 : Spectroscopic &amp; photometric analysis of WDs (Bedard+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/480/1547">J/MNRAS/480/1547 : Full Evolutionary Sequences of Massive WDs (Lauffer+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/878/63">J/ApJ/878/63 : Cool WD atmosphere models. 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in Rad</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL</name><description>[-1.88/3.15] log Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logL</name><description>[0.01/1.4] Uncertainty in logL</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_logtau</name><description>Limit flag on logtau</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</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>SDSS</name><description>SDSS identifier (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>SpT</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>S/N</name><description>[2.2/132.5] Signal-to-Noise</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[30000/150000] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[53/44228] Uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(g)</name><description>[6.42/9.36] log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(g)</name><description>[0.01/1.33] Uncertainty in log(g)</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Atm</name><description>Atmospheric composition</description><ucd>meta.note</ucd></column><column><name>Mass</name><description>[0.23/1.32] Mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>[0.01/0.52] Uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType><flag>nullable</flag></column><column><name>logtau</name><description>[5.0/8.48] log cooling age</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logtau</name><description>[0.01/1.8]? 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