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<ri:Resource created="2022-03-02T13:20:48Z" 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>Color-metallicity relations of GCs. X. M87 spec.</title><shortName>J/ApJS/256/29</shortName><identifier>ivo://CDS.VizieR/J/ApJS/256/29</identifier><altIdentifier>doi:10.26093/cds/vizier.22560029</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kim S.</name></creator><creator><name>Yoon S.-J.</name></creator><creator><name>Lee S.-Y.</name></creator><creator><name>Chung C.</name></creator><creator><name>Sohn S.T.</name></creator><date role="Updated">2022-07-28T07:30:04Z</date><date role="Created">2022-03-02T13:20:48Z</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>globular-star-clusters</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><subject>chemical-abundances</subject><subject>two-color-diagrams</subject><description>We obtained spectra of some 140 globular clusters (GCs) associated with the Virgo central cD galaxy M87 with the Subaru/FOCAS MOS mode. The fundamental properties of GCs such as age, metallicity, and {alpha}-element abundance are investigated by using simple stellar population models. It is confirmed that the majority of M87 GCs are as old as, more metal-rich than, and more enhanced in {alpha}-elements than the Milky Way GCs. Our high-quality, homogeneous data set enables us to test the theoretical prediction of inflected color-metallicity relations (CMRs). The nonlinear-CMR hypothesis entails an alternative explanation for the widely observed GC color bimodality, in which even a unimodal metallicity spread yields a bimodal color distribution by virtue of nonlinear metallicity-to-color conversion. The newly derived CMRs of old, high-signal-to-noise-ratio GCs in M87 (the V-I CMR of 83 GCs and the M-T2 CMR of 78 GCs) corroborate the presence of the significant inflection. Furthermore, from a combined catalog with the previous study on M87 GC spectroscopy, we find that a total of 185 old GCs exhibit a broad, unimodal metallicity distribution. The results corroborate the nonlinear-CMR interpretation of the GC color bimodality, shedding further light on theories of galaxy formation.</description><source format="bibcode">2021ApJS..256...29K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/256/29</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/VII/195">VII/195 : Globular Clusters in the Milky Way (Harris, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/105/1762">J/AJ/105/1762 : Globular clusters around NGC 1399 (Ostrov+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/106/493">J/AJ/106/493 : Globular clusters in M87 (Lee+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/111/377">J/ApJS/111/377 : H{gamma} &amp; H{delta} absorption features (Worthey+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/116/1">J/ApJS/116/1 : Old Stellar Populations. 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