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<ri:Resource created="2019-01-11T12:07:24Z" 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>Hyades tidal tails with Gaia DR2</title><shortName>J/A+A/621/L3</shortName><identifier>ivo://CDS.VizieR/J/A+A/621/L3</identifier><altIdentifier>doi:10.26093/cds/vizier.36219003</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Meingast S.</name></creator><creator><name>Alves J.</name></creator><date role="Updated">2020-04-02T05:00:23Z</date><date role="Created">2019-01-11T12:07:24Z</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>astrometry</subject><description>We report the discovery of two well-defined tidal tails emerging from the Hyades star cluster. The tails were detected in Gaia DR2 data by selecting cluster members in the 3D galactocentric cylindrical velocity space. The robustness of our member selection is reinforced by the fact that the sources depict an almost noiseless, coeval stellar main sequence in the observational Hertzsprung-Russel diagram. The spatial arrangement of the selected members represents a highly flattened shape with respect to the direction of movement along the clusters' orbit in the Galaxy. The size of the entire structure, within the limits of the observations, measures about 200pc in its largest extent, while being only about 25pc thick. This translates into an on-sky extent of well beyond 100deg. Intriguingly, a top-down view on the spatial distribution reveals a distinct S-shape, reminiscent of tidal tails that have been observed for globular clusters and also of tails that were modeled for star clusters bound to the Galactic disk. Even more remarkable, the spatial arrangement as well as the velocity dispersion of our source selection is in excellent agreement with previously published theoretical predictions for the tidal tails of the Hyades. An investigation into observed signatures of equipartition of kinetic energy, that is, mass segregation, remains unsuccessful, most likely because of the sensitivity limit for radial velocity measurements with Gaia.</description><source format="bibcode">2019A&amp;A...621L...3M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/621/L3</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/J/A+A/243/386">J/A+A/243/386 : Hyades members distances (Schwan 1991)</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/A+A/367/111">J/A+A/367/111 : A Hipparcos study of the Hyades cluster (de Bruijne+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/621/L2">J/A+A/621/L2 : Hyades tidal tails revealed by Gaia DR2 (Roeser+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/622/L13">J/A+A/622/L13 : Stellar stream in Gaia DR2 discovery (Meingast+, 2019)</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/A+A/621/L3</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/621/L3</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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