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<ri:Resource created="2015-03-23T10:51:27Z" 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>NGC 5128 globular cluster abundances</title><shortName>J/ApJ/773/L36</shortName><identifier>ivo://CDS.VizieR/J/ApJ/773/L36</identifier><altIdentifier>doi:10.26093/cds/vizier.17739036</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Colucci J.E.</name></creator><creator><name>Duran M.F.</name></creator><creator><name>Bernstein R.A.</name></creator><creator><name>McWilliam A.</name></creator><date role="Updated">2017-06-30T05:49:27Z</date><date role="Created">2015-03-23T10:51:27Z</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>galaxies</subject><subject>radial-velocity</subject><subject>galaxy-kinematics</subject><subject>spectroscopy</subject><description>We present [Fe/H], ages, and Ca abundances for an initial sample of 10 globular clusters in NGC 5128 obtained from high-resolution, high signal-to-noise ratio echelle spectra of their integrated light. All abundances and ages are obtained using our original technique for high-resolution integrated light abundance analysis of globular clusters. The clusters have a range in [Fe/H] between -1.6 and -0.2. In this sample, the average [Ca/Fe] for clusters with [Fe/H]&lt;-0.4 is +0.37+/-0.07, while the average [Ca/Fe] in our Milky Way (MW) and M31 GC samples is +0.29+/-0.09 and +0.24+/-0.10, respectively. This may imply a more rapid chemical enrichment history for NGC 5128 than for either the MW or M31. This sample provides the first quantitative picture of the chemical history of NGC 5128 that is directly comparable to what is available for the MW. Data presented here were obtained with the MIKE echelle spectrograph on the Magellan Clay Telescope.</description><source format="bibcode">2013ApJ...773L..36C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/773/L36</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/AJ/143/84">J/AJ/143/84 : New candidate globular clusters in NGC 5128 (Harris+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/1335">J/ApJ/708/1335 : Spectroscopy of globulars in NGC 5128 (Woodley+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/2101">J/AJ/140/2101 : NGC 5128 globular clusters photometry (Sinnott+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/1871">J/AJ/139/1871 : Kinematics of globulars in NGC 5128 (Woodley+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1533">J/ApJ/705/1533 : NGC 5128 globular clusters (Chattopadhyay+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/704/385">J/ApJ/704/385 : M31 integrated light abundances (Colucci+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/386/1443">J/MNRAS/386/1443 : 2dF study of globular clusters in NGC 5128 (Beasley+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/682/199">J/ApJ/682/199 : Globulars with X-ray sources in NGC 5128 (Woodley+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/494">J/AJ/134/494 : NGC 5128 GCs UBVRICMT1 phot. + RV (Woodley+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/2187">J/AJ/132/2187 : MCT1 photometry of NGC 5128 globular clusters (Harris+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/2140">J/AJ/130/2140 : Abundances and velocities in globular clusters (Pritzl+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/150/367">J/ApJS/150/367 : Globular clusters in NGC 5128 (Peng+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/369/812">J/A+A/369/812 : UVKs phot. of globular clusters in NGC 5128 (Rejkuba, 2001)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/773/L36</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/773/L36</mirrorURL><mirrorURL 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Projected galactocentric radius from NGC 5128 (G1)</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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V-band magnitude from P04 (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[M/H]</name><description>[-1.6/-0.2]? [M/H] metallicity value of Beasley et al. 2008 (J/MNRAS/386/1443)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Z/H]</name><description>[-0.7/1]? [Z/H] metallicity value by W10 (2)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[a/Fe]</name><description>[-0.1/0.3]? [{alpha}/Fe] metallicity value by W10 (2)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vr</name><description>[363/782]? Radial velocity from W07 (G1)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Vr</name><description>[1/34]? Vr uncertainty</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Vs</name><description>[13/24]? Line-of-sight velocity dispersion (v_{sigma}_) measured by Taylor et al. (2010ApJ...712.1191T)</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Vs</name><description>[1/3]? 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