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<ri:Resource created="2014-08-22T11:40:00Z" 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 analysis of NGC 4636 globular clusters</title><shortName>J/ApJ/759/116</shortName><identifier>ivo://CDS.VizieR/J/ApJ/759/116</identifier><altIdentifier>doi:10.26093/cds/vizier.17590116</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Park H.S.</name></creator><creator><name>Lee M.G.</name></creator><creator><name>Hwang H.S.</name></creator><creator><name>Kim S.C.</name></creator><creator><name>Arimoto N.</name></creator><creator><name>Yamada Y.,Tamura N.</name></creator><creator><name>Onodera M.</name></creator><date role="Updated">2017-12-05T05:09:28Z</date><date role="Created">2014-08-22T11:40:00Z</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>globular-star-clusters</subject><subject>spectroscopy</subject><description>We present a spectroscopic analysis of the metallicities, ages, and alpha-elements of the globular clusters (GCs) in the giant elliptical galaxy (gE) NGC 4636 in the Virgo Cluster. Line indices of the GCs are measured from the integrated spectra obtained with Faint Object Camera and Spectrograph on the Subaru 8.2m Telescope. We derive [Fe/H] values of 59 GCs based on the Brodie &amp; Huchra (1990ApJ...362..503B) method, and [Z/H], age, and [{alpha}/Fe] values of 33 GCs from the comparison of the Lick line indices with single stellar population models. The metallicity distribution of NGC 4636 GCs shows a hint of a bimodality with two peaks at [Fe/H]=-1.23({sigma}=0.32) and -0.35({sigma}=0.19). The age spread is large from 2Gyr to 15Gyr and the fraction of young GCs with age &lt;5Gyr is about 27%. The [{alpha}/Fe] of the GCs shows a broad distribution with a mean value [{alpha}/Fe]{approx}0.14dex. The dependence of these chemical properties on the galactocentric radius is weak. We also derive the metallicities, ages, and [{alpha}/Fe] values for the GCs in other nearby gEs (M87, M49, M60, NGC 5128, NGC 1399, and NGC 1407) from the line index data in the literature using the same methods as used for NGC 4636 GCs. The metallicity distribution of GCs in the combined sample of seven gEs including NGC 4636 is found to be bimodal, supported by the KMM test with a significance level of &gt;99.9%. All these gEs harbor some young GCs with ages less than 5Gyr. The mean age of the metal-rich GCs ([Fe/H]&gt;-0.9) is about 3Gyr younger than that of the metal-poor GCs. The mean value of [{alpha}/Fe] of the gE GCs is smaller than that of the Milky Way GCs. We discuss these results in the context of GC formation in gEs.</description><source format="bibcode">2012ApJ...759..116P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/759/116</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/A+A/544/A115">J/A+A/544/A115 : Velocities of NGC 4636 globular clusters (Schuberth+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/377">J/ApJ/709/377 : The globular cluster system of NGC 4636 (Park+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/839">J/MNRAS/405/839 : Spectroscopic obs. of globular clusters (Sharina+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/695/1094">J/ApJ/695/1094 : Chandra observations of NGC 4636 (Posson-Brown+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/459/391">J/A+A/459/391 : Dynamics of NGC 4636 GC system (Schuberth+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/433/43">J/A+A/433/43 : C-T1 phot. of NGC 4636 GC system (Dirsch+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/116/1">J/ApJS/116/1 : Old Stellar Populations. 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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>ID</name><description>[82/10031] Object ID Number (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>L</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[Z/H]1</name><description>? The [Z/H] derived from H{beta} vs. [MgFe]' grid method</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Z/H]1</name><description>? Error of [Z/H]1</description><unit>log(Sun)</unit><ucd>stat.error;src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Z/H]2</name><description>? 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