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<ri:Resource created="2014-06-26T06:40:05Z" status="active" updated="2026-03-18T11:49:00Z" 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>Spectroscopy of NGC 5822-2 and NGC 5822-201</title><shortName>J/AJ/146/39</shortName><identifier>ivo://CDS.VizieR/J/AJ/146/39</identifier><altIdentifier>doi:10.26093/cds/vizier.51460039</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Katime Santrich O.J.</name></creator><creator><name>Pereira C.B.</name></creator><creator><name>de Castro D.B.</name></creator><date role="Updated">2026-03-18T11:49:00Z</date><date role="Created">2014-06-26T06:40:05Z</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>open-star-clusters</subject><subject>barium-stars</subject><subject>line-intensities</subject><description>Open clusters are very useful examples to explain the constraint of the nucleosynthesis process with the luminosities of stars because the distances of the clusters are better known than those of field stars. We carried out a detailed spectroscopic analysis to derive the chemical composition of two red giants in the young open cluster NGC 5822, NGC 5822-2, and NGC 5822-201. We obtained abundances of C, N, O, Na, Mg, Al, Ca, Si, Ti, Ni, Cr, Y, Zr, La, Ce, and Nd. The atmospheric parameters of the studied stars and their chemical abundances were determined using high-resolution optical spectroscopy. We employed the local thermodynamic equilibrium model atmospheres of Kurucz and the spectral analysis code MOOG. The abundances of the light elements were derived using the spectral synthesis technique. We found that NGC 5822-2 and -201 have, respectively, a mean overabundance of the elements created by the s-process, "s," with the notation [s/Fe] of 0.77+/-0.12 and 0.83+/-0.05. These values are higher than those for field giants of similar metallicity. We also found that NGC 5822-2 and -201 have, respectively, luminosities of 140L_{sun}_ and 76L_{sun}_, which are much lower than the luminosity of an asymptotic giant branch star. We conclude that NGC 5822-2 and NGC 5822-201 are two new barium stars first identified in the open cluster NGC 5822. The mass transfer hypothesis is the best scenario to explain the observed overabundances.</description><source format="bibcode">2013AJ....146...39K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/146/39</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/V/81">V/81 : Taxonomy of Barium Stars (Lu 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/108">I/108 : Cape Photographic Durchmusterung (Gill+ 1895-1900)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A51">J/A+A/533/A51 : Abundances of 12 metal-rich barium stars (Pereira+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/515/A28">J/A+A/515/A28 : Abundances of dwarfs &amp; giants in 2 open clusters (Pace+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/502/267">J/A+A/502/267 : EWs of 31 giant stars of 10 open clusters (Smiljanic+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/485/303">J/A+A/485/303 : Radial velocities for 1309 stars &amp; 166 OCl (Mermilliod+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/454/917">J/A+A/454/917 : Abundances of 26 barium stars. II. (Allen+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/81/658">J/AZh/81/658 : Equivalent widths of 9 barium stars (Antipova+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/80/704">J/AZh/80/704 : Studies of classical barium stars (Antipova+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/397/257">J/A+A/397/257 : Chemical compositions of four barium stars (Liang+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/79/909">J/AZh/79/909 : Chemical abundances in barium stars (Boyarchuk+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/319/881">J/A+A/319/881 : Ba II strength of barium stars (Gomez+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/105/78">J/PASP/105/78 : Photometry in open cluster NGC 5822 (Twarog+, 1993)</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/146/39</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/146/39</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/146/39</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/146/39</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/146/39</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/146/39</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/146/39/table1 (Log of the observations and other relevant information for the target stars)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/146/39/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/146/39/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/146/39/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>225.92223333</ra><dec>-54.37578611</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/39345 41834</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/146/39?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/AJ/146/39/table1</name><description>Log of the observations and other relevant information for the target stars</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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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>Ion</name><description>Iron line identifier (FeI or FeII)</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>lambda</name><description>Wavelength; in {AA}</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LEP</name><description>Lower excitation potential of the transition</description><unit>eV</unit><ucd>phys.atmol.excitation;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggf</name><description>Log of the oscillator strength (1)</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EW2</name><description>? 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