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<ri:Resource created="2004-12-03T21:34:03Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Elemental abundances of 3 red giants in Ter 7</title><shortName>J/AJ/127/373</shortName><identifier>ivo://CDS.VizieR/J/AJ/127/373</identifier><altIdentifier>doi:10.26093/cds/vizier.51270373</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tautvaisiene G.</name></creator><creator><name>Wallerstein G.</name></creator><creator><name>Geisler D.</name></creator><creator><name>Gonzalez G.</name></creator><creator><name>Charbonnel C.</name></creator><date role="Updated">2023-04-06T16:51:05Z</date><date role="Created">2004-12-03T21:34:03Z</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>chemically-peculiar-stars</subject><description>Chemical abundances in three giants in Terzan 7, a globular cluster associated with the Sagittarius dwarf galaxy, have been determined using high-resolution spectra obtained with the UVES spectrograph on the ESO 8.2m Kueyen telescope. We find the overall metallicity of the stars to be [Fe/H]=-0.61+/-0.07, which is slightly higher than that previously evaluated from photometry and used for the age determination of this cluster. This metallicity yields an age of about 6Gyr, which is slightly lower than derived from previous estimates. The relative abundance ratios of various chemical elements to iron lie between those of its host galaxy's metal-poor and metal-rich stars and reveal an intriguing similarity to the pattern seen in the Large Magellanic Cloud.</description><source format="bibcode">2004AJ....127..373T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/127/373</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/AJ/127/373</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/127/373</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/127/373</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/127/373</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/127/373</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/127/373</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/127/373/table1</name><description>Equivalent Widths of Spectral Lines of Three Red Giants in Terzan 7</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Element</name><description>Line identification (1)</description><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lambda</name><description>Wavelength in angstroms</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S16-EW</name><description>? Cl* terzan 7 SL 16 equivalent width (2)</description><unit>pm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S34-EW</name><description>? Cl* terzan 7 SL 34 equivalent width (2)</description><unit>pm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S35-EW</name><description>? Cl* terzan 7 SL 35 equivalent width (2)</description><unit>pm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>