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<ri:Resource created="2021-04-16T09:26:50Z" 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>Disentangling cataclysmic variables in Gaia DR2</title><shortName>J/MNRAS/492/L40</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/492/L40</identifier><altIdentifier>doi:10.26093/cds/vizier.74929040</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Abril J.</name></creator><creator><name>Schmidtobreick L.</name></creator><creator><name>Ederoclite A.</name></creator><creator><name>Lopez-Sanjuan C.</name></creator><date role="Updated">2024-08-20T20:16:03Z</date><date role="Created">2021-04-16T09:26:50Z</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>cataclysmic-variable-stars</subject><subject>stellar-distance</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>proper-motions</subject><subject>apparent-magnitude</subject><description>Cataclysmic Variables (CVs) are interacting binaries consisting of at least three components that control their colour and magnitude. Using Gaia we here investigate the influence of the physical properties of these binaries on their position in the Hertzsprung-Russell diagram (HR-diagram). The CVs are on average located between the main sequence and the white dwarf regime, the maximum density being at G_BP_-G_RP_~=0.56 and G_abs_~10.15. We nd a trend of the orbital period with colour and absolute brightness: with decreasing period, the CVs become bluer and fainter. We also identify the location of the various CV sub-types in the HR-diagram and discuss the possible location of detached CVs, going through the orbital period gap.</description><source format="bibcode">2020MNRAS.492L..40A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/492/L40</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/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/V/123">V/123 : Catalog of Cataclysmic Variables (Downes+ 2001-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/cb">B/cb : Cataclysmic Binaries, LMXBs, and related objects (Ritter+, 2004)</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/492/L40</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/492/L40</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/492/L40</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/492/L40</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/492/L40</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/492/L40</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/492/L40/catalog (Crossmatch of CVs with Gaia's parallaxes and Bailer-Jones (Cat. 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Gaia DR2 Parallax (parallax)</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_plx</name><description>? Gaia DR2 Standard error of parallax (parallax_error)</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmRA</name><description>? Gaia DR2 Proper motion in right ascension direction, pmRA*cosDE (yr pmra)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_pmRA</name><description>? Gaia DR2 Standard error of proper motion in right ascension direction (pmra_error)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmDE</name><description>? 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Gaia DR2 Stellar effective temperature (teff_val)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CATS</name><description>Display Gaia and CV original data</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Apparent magnitude at maximum brightness from CV catalog (B/cb) (mag1)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Orb.Per</name><description>Orbital period from CV catalog (B/cb) (Orb.Per)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Outburst</name><description>? Year of outburst from CV catalog (V/123) (Outburst)</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MagRange</name><description>Magnitude range from CV catalog (V/123) (Mag.Range)</description><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>SpType2</name><description>Spectral type of the secondary from CV catalog (B/cb) (SpType2)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>SpType1</name><description>Spectral type of the primary from CV catalog (B/cb) (SpType1)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Source</name><description>Gaia source identifier, identical to the Gaia-DR2 source_id. 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