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<ri:Resource created="2026-06-12T13:42:35Z" status="active" updated="2026-06-12T12:45:39Z" 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>[M/H] of K/M dwarfs in SN kinematic structures</title><shortName>J/MNRAS/521/208</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/521/208</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Medan I.</name></creator><creator><name>Lepine S.</name></creator><date role="Updated">2026-06-12T12:45:39Z</date><date role="Created">2026-06-12T13:42:35Z</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>k-stars</subject><subject>dwarf-stars</subject><subject>milky-way-galaxy</subject><subject>chemical-abundances</subject><subject>stellar-associations</subject><subject>astrometry</subject><description>We combine photometric metallicities with astrometry from Gaia DR3 to examine the chemodynamic structure of ~250000 K dwarfs in the solar neighbourhood (SN). In kinematics, we observe ridges/clumps of 'kinematic groups', like studies of more massive main-sequence stars. Here, we note clear differences in both metallicity and vertical velocity as compared with the surrounding regions in velocity space and hypothesize this is due to differences in mean age. To test this, we develop a method to estimate the age distribution of subpopulations of stars. In this method, we use GALAH data to define probability distributions of W versus [M/H] in age bins of 2 Gyr and determine optimal age distributions as the best-fitting weighted sum of these distributions. This process is then validated using the GALAH subset. We estimate the probable age distribution for regions in the kinematic plane, where we find significant substructure that is correlated with the kinematic groups. Most notably, we find an age gradient across the Hercules streams that is correlated with birth radius. Finally, we examine the bending and breathing modes as a function of age. From this, we observe potential hints of an increase in the bending amplitude with age, which will require further analysis in order to confirm it. This is one of the first studies to examine these chemodynamics in the SN using primarily low-mass stars and we hope these findings can better constrain dynamical models of the Milky Way due to the increase in resolution the sample size provides.</description><source format="bibcode">2023MNRAS.521..208M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/521/208</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/J/MNRAS/506/150">J/MNRAS/506/150 : The GALAH+ Survey DR3 (Buder+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/478/3809">J/MNRAS/478/3809 : TGAS distances (Schonrich+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/473/2004">J/MNRAS/473/2004 : TESS-HERMES Survey Data Release 1 catalog (Sharma+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/440/3430">J/MNRAS/440/3430 : SDSS-2MASS-WISE stellar colour locus (Davenport+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/669/A104">J/A+A/669/A104 : Stellar parameters from Gaia DR3 (Kordopatis+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/619/A72">J/A+A/619/A72 : Milky Way disk kinematic sub-structures (Ramos+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/430/165">J/A+A/430/165 : Radial velocities for 6691 K and M giants (Famaey+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/234">J/AJ/161/234 : 1.7 million K and M dwarfs cross-matching (Medan+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/694">J/AJ/133/694 : Abundances in the HR 1614 moving group (De Silva+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : 2MASS All-Sky Extended Source Catalog (XSC)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/117">V/117 : Geneva-Copenhagen Survey of Solar neighbourhood</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/286">III/286 : APOGEE-2 DR17 final allStar catalog (Abdurro'uf+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+,2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><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/I/355">I/355 : Gaia DR3 Part 1. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GaiaDR3</name><description>The GaiaDR3 source ID (source_id)</description><ucd>meta.id;meta.main</ucd></column><column><name>2M-AllWISE-PS1</name><description>Display the 2MASS, AllWISE and Pan-STARRS data linked</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>U</name><description>Galactic U velocity (U)</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>[M/H]</name><description>Photometric metallicity estimated with calibrated relationship from Medan et al. 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