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<ri:Resource created="2011-04-29T16:19:24Z" 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>Arp 2 and Ter 8 red giants equivalent widths</title><shortName>J/AJ/136/614</shortName><identifier>ivo://CDS.VizieR/J/AJ/136/614</identifier><altIdentifier>doi:10.26093/cds/vizier.51360614</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mottini M.</name></creator><creator><name>Wallerstein G.</name></creator><creator><name>McWilliam A.</name></creator><date role="Updated">2017-06-26T11:48:54Z</date><date role="Created">2011-04-29T16:19:24Z</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>giant-stars</subject><subject>line-intensities</subject><subject>effective-temperature</subject><description>To compare the globular clusters (GCs) associated with the Sagittarius Galaxy (Sgr) we report the results obtained from new high-resolution spectra of red giant stars in Terzan 8 and Arp 2, collected with the Magellan Inamori Kyocera Echelle (MIKE) spectrograph at Las Campanas Observatory.</description><source 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