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<ri:Resource created="2023-11-22T09:54:13Z" status="active" updated="2025-06-13T15:25:00Z" 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>Pleiades members &amp; escapee candidates with Gaia EDR3</title><shortName>J/ApJ/926/132</shortName><identifier>ivo://CDS.VizieR/J/ApJ/926/132</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Heyl J.</name></creator><creator><name>Caiazzo I.</name></creator><creator><name>Richer H.B.</name></creator><date role="Updated">2023-11-22T08:57:02Z</date><date role="Created">2023-11-22T09:54:13Z</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>open-star-clusters</subject><subject>apparent-magnitude</subject><subject>visible-astronomy</subject><subject>astrometry</subject><subject>two-color-diagrams</subject><description>We search through an eight million cubic parsec volume surrounding the Pleiades star cluster and the Sun to identify both the current and past members of the Pleiades cluster within the Gaia EDR3 data set. We find nearly 1300 current cluster members and 289 former cluster candidates. Many of these candidates lie well in front of or behind the cluster from our point of view, so formerly they were considered cluster members, but their parallaxes put them more than 10pc from the center of the cluster today. Over the past 100Myr we estimate that the cluster has lost twenty percent of its mass including two massive white dwarf stars and the {alpha}^2^ Canum Venaticorum type variable star, 41 Tau. All three white dwarfs associated with the cluster are massive (1.01-1.06M _{sun}_) and have progenitors with main-sequence masses of about six solar masses. Although we did not associate any giant stars with the cluster, the cooling time of the oldest white dwarf of 60Myr gives a firm lower limit on the age of the cluster.</description><source format="bibcode">2022ApJ...926..132H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/926/132</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/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/331/81">J/A+A/331/81 : Hyades membership (Perryman+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/1221">J/AJ/132/1221 : VJHK and SDSS photometry of DA white dwarfs (Holberg+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/138">J/ApJ/743/138 : Spectroscopic survey of bright white dwarfs (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/ApJ/758/56">J/ApJ/758/56 : Young M dwarfs within 25pc. II. Kinematics (Shkolnik+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/A10">J/A+A/616/A10 : 46 open clusters GaiaDR2 HR diag. (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/623/A35">J/A+A/623/A35 : A 3D view of the Hyades population (Lodieu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/628/A66">J/A+A/628/A66 : alpha Persei, Pleiades and Praesepe clusters (Lodieu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/901/93">J/ApJ/901/93 : Model atm. analysis of hot WDs from SDSS DR12 (Bedard+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/638/A131">J/A+A/638/A131 : Radial velocities of 643 DA white dwarfs (Napiwotzki+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/645/A84">J/A+A/645/A84 : Coronae of nearby star clusters (Meingast+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/912/165">J/ApJ/912/165 : Massive white dwarfs in young star clusters (Richer+, 2021)</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/ApJ/926/132</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/926/132</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/926/132</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/926/132</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/926/132</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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