<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2009-12-27T18:18:31Z" 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>Lithium in globular NGC 6397</title><shortName>J/A+A/505/L13</shortName><identifier>ivo://CDS.VizieR/J/A+A/505/L13</identifier><altIdentifier>doi:10.26093/cds/vizier.35059013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gonzalez Hernandez J.I.</name></creator><creator><name>Bonifacio P.</name></creator><creator><name>Caffau E.</name></creator><creator><name>Steffen M.</name></creator><creator><name>Ludwig H.-G.,Behara N.T.</name></creator><creator><name>Sbordone L.</name></creator><creator><name>Cayrel R.</name></creator><creator><name>Zaggia S.</name></creator><date role="Updated">2009-12-27T17:26:44Z</date><date role="Created">2009-12-27T18:18:31Z</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>dwarf-stars</subject><subject>giant-stars</subject><subject>line-intensities</subject><subject>effective-temperature</subject><description>Most globular clusters are believed to host a single stellar population. They can thus be considered a good place to study the Spite plateau and to search for possible evolutionary modifications of the Li content. We want to determine the Li content of subgiant (SG) and main sequence (MS) stars of the old, metal-poor globular cluster NGC 6397. This work was aimed not only at studying possible Li abundance variations but also to investigate the cosmological Li discrepancy.</description><source format="bibcode">2009A&amp;A...505L..13G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/505/L13</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/287/769">J/A+A/287/769 : UV photometry of NGC 6397 (Burgarella+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/106/404">J/PASP/106/404 : NGC 6535 BV CCD photometry (Sarajedini, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/99/637">J/ApJS/99/637 : Equivalent widths for 54 red giants (Norris+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/108/682">J/PASP/108/682 : Low-Mass Stars in Outer Field in NGC 6397 (Mould+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/122/1">J/A+AS/122/1 : BV photometry of variables in NGC 6397 (Kaluzny, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/425/509">J/A+A/425/509 : VI photometry of NGC 6397 (Andreuzzi+, 2004)</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/A+A/505/L13</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/505/L13</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/505/L13</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/505/L13</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/505/L13</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/505/L13</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/A+A/505/L13/table2 (Effective temperature, Equivalent Width and Li abundances in stars of NGC 6397)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/505/L13/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/505/L13/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/505/L13/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>265.1280417</ra><dec>-53.7944167</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/42076</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/505/L13?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/505/L13/table2</name><description>Effective temperature, Equivalent Width and Li abundances in stars of NGC 6397</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Name of the star (MSSNNNNNN or SGBNNNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Vmag</name><description>V magnitude in the Johnson system</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B-V</name><description>? B-V magnitude in the Johnson system</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNR</name><description>Signal-to-noise ratio (1)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff(3D)</name><description>3D H{alpha}-based Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective;spect.line</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff(1D)</name><description>1D H{alpha}-based Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective;spect.line</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>EW</name><description>Equivalent width of Li 6708 line (in m{AA})</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_EWa</name><description>rms uncertainty in the equivalent width measurements estimated from a fitting routine (2)</description><unit>0.1pm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_EWb</name><description>rms uncertainty in the equivalent width associated to S/N ratio and dispersion of the spectra (3)</description><unit>0.1pm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>A(Li)</name><description>3D,NLTE Li abundance (log scale, H=12)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>