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<ri:Resource created="2023-05-12T07:20:55Z" 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>Chemical abundances in binary stars</title><shortName>J/ApJ/920/94</shortName><identifier>ivo://CDS.VizieR/J/ApJ/920/94</identifier><altIdentifier>doi:10.26093/cds/vizier.19200094</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Espinoza-Rojas F.,Chaname J.,Jofre P.,Casamiquela L.</name></creator><date role="Updated">2024-06-07T16:01:06Z</date><date role="Created">2023-05-12T07:20:55Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>chemical-abundances</subject><description>The abundance ratios of some chemical species have been found to correlate with stellar age, leading to the possibility of using stellar atmospheric abundances as stellar age indicators. These chemical clocks have already been calibrated with solar twins and open clusters, but it remains to be seen whether they can be effective at identifying coeval stars in a population that spans a broad parameter space (i.e., the promise of chemical tagging). Since the components of wide binaries are known to be stars of common origins, they constitute ideal laboratories for testing the usefulness of chemical clocks for the age dating of field stars. Using a combination of our new measurements and literature data on wide binaries, we show for the first time that chemical clocks are even more consistent among the components of wide binaries than their individual abundances. Moreover, the special case of HIP 34426/HIP 34407 may indicate that chemical clocks are consistent for coeval stars even when those individual abundances are not. If the assumption that chemical clocks are reliable age indicators is correct, this would constitute the first statistically significant evidence that the components of wide binaries are indeed coeval, validating a large body of published work that relies on that to be the case. Furthermore, our results provide strong evidence that chemical clocks indeed carry important information about stellar birthplaces and chemical evolution, and thus we propose that including them in chemical tagging efforts may facilitate the identification of now-dissolved stellar groups.</description><source format="bibcode">2021ApJ...920...94E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/920/94</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/ApJS/150/455">J/ApJS/150/455 : New HIP-based parallaxes for 424 faint stars (Gould+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/441/1149">J/A+A/441/1149 : Abundances of 20 F-G disk stars (del Peloso+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/454/581">J/A+A/454/581 : Iron abundances of 33 wide binaries (Desidera+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/704/531">J/ApJ/704/531 : The coevality of young binary systems (Kraus+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/508/L17">J/A+A/508/L17 : Abundances in solar analogs (Ramirez+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/577/A9">J/A+A/577/A9 : Sc, V, Mn, and Co in Milky Way stars (Battistini+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/582/A81">J/A+A/582/A81 : Gaia FGK benchmark stars; 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HIP15304 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP15310</name><description>? HIP15310 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP32865</name><description>? HIP32865 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP32871</name><description>? HIP32871 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP34407</name><description>? HIP34407 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP34426</name><description>? HIP34426 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP52792</name><description>? HIP52792 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP52793</name><description>? HIP52793 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP58240</name><description>? HIP58240 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HIP58241</name><description>? HIP58241 equivalent width; m{AA}</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/920/94/refs</name><description>References used for tablea2 and tablea3</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>Ref</name><description>Reference code</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>BIB</name><description>BIBcode of the reference</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Cat.</name><description>Vizier catalog</description><ucd>meta.id;meta.table</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>Note</name><description>Additional note or comment</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="95*">char</dataType></column></table></schema></tableset></ri:Resource>