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<ri:Resource created="2020-11-05T07:54:37Z" 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>Stellar parameters for 13196 Kepler dwarfs</title><shortName>J/AJ/160/90</shortName><identifier>ivo://CDS.VizieR/J/AJ/160/90</identifier><altIdentifier>doi:10.26093/cds/vizier.51600090</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Angus R.</name></creator><creator><name>Beane A.</name></creator><creator><name>Price-Whelan A.M.</name></creator><creator><name>Newton E.</name></creator><creator><name>Curtis J.L.</name></creator><creator><name>Berger T.,van Saders J.</name></creator><creator><name>Kiman R.</name></creator><creator><name>Foreman-Mackey D.</name></creator><creator><name>Lu Y.</name></creator><creator><name>Anderson L.</name></creator><creator><name>Faherty J.K.</name></creator><date role="Updated">2021-09-22T07:28:11Z</date><date role="Created">2020-11-05T07:54:37Z</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>dwarf-stars</subject><subject>stellar-masses</subject><subject>effective-temperature</subject><subject>galaxy-kinematics</subject><subject>visible-astronomy</subject><description>The rotational evolution of cool dwarfs is poorly constrained after ~1-2Gyr due to a lack of precise ages and rotation periods for old main-sequence stars. In this work, we use velocity dispersion as an age proxy to reveal the temperature-dependent rotational evolution of low-mass Kepler dwarfs and demonstrate that kinematic ages could be a useful tool for calibrating gyrochronology in the future. We find that a linear gyrochronology model, calibrated to fit the period-Teff relationship of the Praesepe cluster, does not apply to stars older than around 1Gyr. Although late K dwarfs spin more slowly than early-K dwarfs when they are young, at old ages, we find that late K dwarfs rotate at the same rate or faster than early-K dwarfs of the same age. This result agrees qualitatively with semiempirical models that vary the rate of surface-to-core angular momentum transport as a function of time and mass. It also aligns with recent observations of stars in the NGC6811 cluster, which indicate that the surface rotation rates of K dwarfs go through an epoch of inhibited evolution. We find that the oldest Kepler stars with measured rotation periods are late K and early M dwarfs, indicating that these stars maintain spotted surfaces and stay magnetically active longer than more massive stars. Finally, based on their kinematics, we confirm that many rapidly rotating GKM dwarfs are likely to be synchronized binaries.</description><source format="bibcode">2020AJ....160...90A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/160/90</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/III/198">III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/117">V/117 : Geneva-Copenhagen Survey of Solar neighbourhood (Holmberg+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/137">VI/137 : GaiaSimu Universe Model Snapshot (Robin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/426">J/AJ/128/426 : Subdwarfs in the SDSS (West+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/377/741">J/MNRAS/377/741 : VIc photometry of NGC 2516 (Irwin+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2258">J/AJ/133/2258 : Activity and kinematics of ultracool dwarfs (Schmidt+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/1264">J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/785">J/AJ/135/785 : SDSS-DR5 low-mass star spectroscopic sample (West+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/1">J/AJ/137/1 : PMs and astrometry of late-type dwarfs (Faherty+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A138">J/A+A/530/A138 : Geneva-Copenhagen survey re-analysis (Casagrande+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/92">J/AJ/141/92 : BVI photometry of 10 distant open clusters (Janes+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/L9">J/ApJ/733/L9 : Stellar rotation for 71 NGC 6811 members (Meibom+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. 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