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<ri:Resource created="2023-07-20T10:19:14Z" status="active" updated="2026-07-01T14:00:44Z" 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>Rotation of wide binaries</title><shortName>J/A+A/675/A180</shortName><identifier>ivo://CDS.VizieR/J/A+A/675/A180</identifier><altIdentifier>doi:10.26093/cds/vizier/bc-n3/lbia</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gruner D.</name></creator><creator><name>Barnes S.A.</name></creator><creator><name>Janes K.A.</name></creator><date role="Updated">2026-07-01T14:00:44Z</date><date role="Created">2023-07-20T10:19:14Z</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>multiple-stars</subject><subject>late-type-stars</subject><subject>variable-stars</subject><subject>stellar-ages</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Gyrochronology allows the derivation of ages of late-type main sequence stars from their rotation periods and a mass proxy such as color. It has been explored in open clusters, but a connection to field stars has yet to be established successfully. We explore the rotation rates of wide binaries, representing enlightening intermediaries between clusters and field stars, and their overlap with those of open cluster stars. We investigate a recently created catalog of wide binaries, match them to observations by the Kepler mission (and its K2 extension), validate or rederive their rotation periods, identify 283 systems where both stars are on the main sequence and have vetted rotation periods, and compare them with open cluster data. We find that the vast majority of these wide binaries (236) line up directly along the curvilinear ribs defined by open clusters in color-period diagrams or along the equivalent interstitial gaps between successive open clusters. The parallelism in shape is remarkable. 12 additional systems are clearly rotationally older. The deviant systems, a minority, are mostly demonstrably hierarchical. Furthermore, the position in the color-magnitude diagram of the evolved component in the additional wide binary systems containing one is consistent with the main sequence component's rotational age.</description><source format="bibcode">2023A&amp;A...675A.180G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/675/A180</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/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (KIC) (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1 (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/635/A43">J/A+A/635/A43 : Stellar rotation periods from K2 Campaigns 0-18</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/675/A180</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/675/A180</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Gaia DR3 radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_RV</name><description>? Error on Gaia DR3 radial velocity</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProtMQ14</name><description>? Rotation period in MQ14 [d]</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_ProtMQ14</name><description>? Error on Rotation period in MQ14</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProtRH20</name><description>? 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