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<ri:Resource created="2017-11-13T11:31:19Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" 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/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>Asteroseismology for solar analogues 16 Cyg A/B</title><shortName>J/MNRAS/446/2959</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/446/2959</identifier><altIdentifier>doi:10.26093/cds/vizier.74462959</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Davies G.R.</name></creator><creator><name>Chaplin W.J.</name></creator><creator><name>Farr W.M.</name></creator><creator><name>Garcia R.A.</name></creator><creator><name>Lund M.N.</name></creator><creator><name>Mathis S.,Metcalfe T.S.</name></creator><creator><name>Appourchaux T.</name></creator><creator><name>Basu S.</name></creator><creator><name>Benomar O.</name></creator><creator><name>Campante T.L.,Ceillier T.</name></creator><creator><name>Elsworth Y.</name></creator><creator><name>Handberg R.</name></creator><creator><name>Salabert D.</name></creator><creator><name>Stello D.</name></creator><date role="Updated">2024-08-14T20:18:57Z</date><date role="Created">2017-11-13T11:31:19Z</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>g-stars</subject><subject>multiple-stars</subject><description>The solar analogues 16 Cyg A and B are excellent asteroseismic targets in the Kepler field of view and together with a red dwarf and a Jovian planet form an interesting system. For these more evolved Sun-like stars we cannot detect surface rotation with the current Kepler data but instead use the technique of asteroseismology to determine rotational properties of both 16 Cyg A and B. We find the rotation periods to be 23.8^1.5^_-1.8_ and 23.2^11.5^_-3.2_ d, and the angles of inclination to be 56^6^_-5_ {deg} and 36^17^_-7_ {deg}, for A and B, respectively. Together with these results we use the published mass and age to suggest that, under the assumption of a solar-like rotation profile, 16 Cyg A could be used when calibrating gyrochronology relations. In addition, we discuss the known 16 Cyg B star-planet eccentricity and measured low obliquity which is consistent with Kozai cycling and tidal theory.</description><source format="bibcode">2015MNRAS.446.2959D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/446/2959</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/737/L32">J/ApJ/737/L32 : Abundances of 16 Cyg A and B (Schuler+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/790/L23">J/ApJ/790/L23 : Solar analogs and twins rotation by Kepler</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/446/2959</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/446/2959</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/446/2959</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/446/2959</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/446/2959</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/446/2959</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/446/2959/tables12</name><description>Mode frequencies for 16 Cyg A (tables1) and 16 Cyg B (tables2) with 68% credible regions</description><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>16Cyg</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>n</name><description>[12/27] Radial order n</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l</name><description>[0/3] The degree l of the mode</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Freq</name><description>Frequency</description><unit>1e-06Hz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Region</name><description>The 68% credible region</description><unit>1e-06Hz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>