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<ri:Resource created="2024-04-12T13:48:54Z" 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>Ages, masses &amp; kinematics of GALAH MS turnoff stars</title><shortName>J/ApJ/929/124</shortName><identifier>ivo://CDS.VizieR/J/ApJ/929/124</identifier><altIdentifier>doi:10.26093/cds/vizier.19290124</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen X.</name></creator><creator><name>Ge Z.</name></creator><creator><name>Chen Y.</name></creator><creator><name>Bi S.</name></creator><creator><name>Yu J.</name></creator><creator><name>Yang W.</name></creator><creator><name>Ferguson J.W.</name></creator><creator><name>Wu Y.,Li Y.</name></creator><date role="Updated">2024-11-06T20:24:46Z</date><date role="Created">2024-04-12T13:48:54Z</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>chemical-abundances</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>surveys</subject><subject>milky-way-galaxy</subject><subject>astronomical-models</subject><subject>visible-astronomy</subject><description>Main-sequence turnoff (MSTO) stars are good tracers of Galactic populations since their ages can be reliably estimated from atmospheric parameters. Based on the GALAH survey, we use the Yale rotation evolution code to determine the ages of 2926 MSTO stars with a mean age uncertainty of ~10% considering the variation of C and O abundances. The ages of CO-poor stars are systematically affected by ~10% due to the C and O abundances, globally shifting to ~0.5Gyr older compared to the results using solar metal mixture. Of the stars with [Fe/H]~0.3-0.5 or [O/Fe]&lt;=-0.25, many have fractional age differences of &gt;=20%, and even reach up to 36%. The age-metallicity relation appears to possibly indicate the existence of two distinct sequences: a young sequence of stars with ages mostly &lt;7Gyr, and a relatively older sequence of stars with ages mostly &gt;7Gyr, overlapping at 5Gyr&lt;=age&lt;=7Gyr. Moreover, the trends of abundances-to-age ratios show two corresponding sequences, especially in the [O/Fe]-age plane. We also find that [Y/Mg] is a good chemical clock in disk populations. The young sequence and the old sequence cannot be separated based on chemistry or kinematics; therefore, stellar age is an important parameter to distinguish these two sequences in our sample.</description><source format="bibcode">2022ApJ...929..124C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/929/124</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/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/433/185">J/A+A/433/185 : Abundance analysis of 102 F and G dwarfs (Bensby+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/367/1329">J/MNRAS/367/1329 : Elemental abundances for 176 stars (Reddy+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/545/A32">J/A+A/545/A32 : Chemical abundances of 1111 FGK stars (Adibekyan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A71">J/A+A/562/A71 : Abundances of solar neighbourhood dwarfs (Bensby+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A25">J/A+A/568/A25 : C and O abundances in stellar populations (Nissen+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/576/A89">J/A+A/576/A89 : O abundances from HARPS in F-G stars (Bertran de Lis+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/608/A112">J/A+A/608/A112 : Kepler LEGACY stars high-precision abund. (Nissen+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/475/5487">J/MNRAS/475/5487 : Stellar properties of KIC stars (Silva Aguirre+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/630/A104">J/A+A/630/A104 : Disk and halo stars C, O and Fe abundances (Amarsi+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/624/A19">J/A+A/624/A19 : GALAH chemodynamical analyse with TGAS (Buder+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/624/A78">J/A+A/624/A78 : Masses &amp; ages of 1059 HARPS-GTO stars (Delgado Mena+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/621/A112">J/A+A/621/A112 : Carbon and oxygen in 107 dwarf stars (Pavlenko+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/639/A127">J/A+A/639/A127 : Age-chemical-clocks-metallicity relations (Casali+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/889/157">J/ApJ/889/157 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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>P</name><description>Display the fundamental and kinematic parameters determined in this work (link to Table 6)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>2MASS</name><description>GALAH DR3 star identifier (HHMMSSss+DDMMSSs; J2000) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType><flag>primary</flag></column><column><name>Teff</name><description>[5600/6875]? Surface effective temperature (1)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Teff</name><description>[69/79]? Uncertainty in Teff (1)</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logg</name><description>[3.8/4.3]? log, Surface gravity (1)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logg</name><description>[0.06/0.3]? Uncertainty in logg (1)</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FeH</name><description>[-0.6/0.6] Metallicity, [Fe/H] (1)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FeH</name><description>[0.04/0.05]? Uncertainty in Fe/H (1)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[C/H]</name><description>[-0.5/0.6] Carbon abundance (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>[O/H]</name><description>[-1.2/0.7]? Oxygen abundance (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[a/Fe]</name><description>[-0.7/0.6] {alpha} element abundance, relative to Fe (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>_RA</name><description>Positions from 2MASS identifiers (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from 2MASS identifiers (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/929/124/table6</name><description>Fundamental and kinematic parameters for the whole determined in this work; updated version</description><column><name>2MASS</name><description>GALAH DR3 star identifier as in Table 1 (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><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>Mstar</name><description>[0.8/1.5] Stellar mass, derived with CO-mixtures</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mstar</name><description>[-0.1/0] Lower uncertainty for Mstar</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_Mstar</name><description>[0/0.1] Upper uncertainty for Mstar</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AgeCO</name><description>[1.2/13.5] Age, derived with CO-mixtures</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_AgeCO</name><description>[-1.4/-0.007] Lower uncertainty for AgeCO</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_AgeCO</name><description>[0.006/2.1] Upper uncertainty for AgeCO</description><unit>Gyr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age</name><description>[1.2/13.5] Age, derived with GS98 solar-mixture or alpha-enhanced mixtures</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Age</name><description>[-1.5/-0.002] Lower uncertainty for Age</description><unit>Gyr</unit><ucd>stat.error;time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Age</name><description>[0.006/2.1] Upper uncertainty for Age</description><unit>Gyr</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>U</name><description>[-141/105]? LSR U space motion</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.x;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>V</name><description>[-132/51]? LSR V space motion</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.y;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>W</name><description>[-80/69]? LSR W space motion</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>