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<ri:Resource created="2016-03-21T15:28:30Z" 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>M62 (NGC 6266) giant branch stars abundances</title><shortName>J/ApJ/813/97</shortName><identifier>ivo://CDS.VizieR/J/ApJ/813/97</identifier><altIdentifier>doi:10.26093/cds/vizier.18130097</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lapenna E.</name></creator><creator><name>Mucciarelli A.</name></creator><creator><name>Ferraro F.R.</name></creator><creator><name>Origlia L.</name></creator><creator><name>Lanzoni B.,Massari D.</name></creator><creator><name>Dalessandro E.</name></creator><date role="Updated">2018-01-08T06:58:08Z</date><date role="Created">2016-03-21T15:28:30Z</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>chemical-abundances</subject><subject>radial-velocity</subject><subject>giant-stars</subject><description>We have collected UVES-FLAMES high-resolution spectra for a sample of 6 asymptotic giant branch (AGB) and 13 red giant branch (RGB) stars in the Galactic globular cluster (GC) M62 (NGC 6266). Here we present the detailed abundance analysis of iron, titanium, and light elements (O, Na, Mg, and Al). For the majority (five out of six) of the AGB targets, we find that the abundances of both iron and titanium determined from neutral lines are significantly underestimated with respect to those obtained from ionized features, the latter being, instead, in agreement with those measured for the RGB targets. This is similar to recent findings in other clusters and may suggest the presence of nonlocal thermodynamic equilibrium (NLTE) effects. In the O-Na, Al-Mg, and Na-Al planes, the RGB stars show the typical correlations observed for GC stars. Instead, all the AGB targets are clumped in the regions where first-generation stars are expected to lie, similar to what was recently found for the AGB population of NGC6752. While the sodium and aluminum abundances could be underestimated as a consequence of the NLTE bias affecting iron and titanium, the oxygen line used does not suffer from the same effects, and the lack of O-poor AGB stars therefore is a solid result. We can thus conclude that none of the investigated AGB stars belongs to the second stellar generation of M62. We also find an RGB star with extremely high sodium abundance ([Na/Fe]=+1.08dex).</description><source format="bibcode">2015ApJ...813...97L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/813/97</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/ApJ/801/69">J/ApJ/801/69 : Iron EWs for NGC3201 giant star members (Mucciarelli+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A60">J/A+A/564/A60 : NGC 4833 Na-O measured with FLAMES (Carretta+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/27">J/ApJS/208/27 : Sun and HD 84937 TiII log(gf) and abundances (Wood+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/775/L27">J/ApJ/775/L27 : Chemical abundances in a metal-poor RGB star (Johnson+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/A128">J/A+A/557/A128 : Stellar [Fe/H] and [Na/H] in NGC6752 (Carretta, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/498.198">J/other/Nat/498.198 : Na abundances in NGC6752 (Campbell+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/70">J/AJ/143/70 : Differential reddening in MW globulars (Alonso-Garcia+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/L38">J/ApJ/754/L38 : Abundances &amp; radial velocities of M13 giants (Johnson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/91">J/ApJ/750/91 : Metallicities of old stellar systems (Chattopadhyay+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A80">J/A+A/534/A80 : Bulge clump giant metallicity in Baade's window (Hill+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/64">J/ApJ/731/64 : Spectroscopy of 300 RGBs in {omega} Cen (Marino+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/839">J/MNRAS/405/839 : Spectroscopic obs. of globular clusters (Sharina+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/139">J/A+A/505/139 : Abundances of red giants in 17 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/117">J/A+A/505/117 : Abundances of red giants in 15 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/695/L134">J/ApJ/695/L134 : Chemical anomalies in old LMC clusters (Mucciarelli+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/177">J/A+A/486/177 : Bulge field stars from FLAMES-GIRAFFE sp. 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temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[0.8/1.6] Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vturb</name><description>[1.3/1.8] Microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[FeI/H]</name><description>[-1.3/-1] Abundance of [FeI/H]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeI/H]</name><description>[0.01] [FeI/H] internal uncertainty</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nFeI</name><description>[102/146] Number of FeI lines used</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[FeII/H]</name><description>[-1.2/-0.9] Abundance of [FeII/H]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeII/H]</name><description>[0.01/0.04] [FeII/H] internal uncertainty</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nFeII</name><description>[7/12] Number of FeII lines used</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[TiI/H]</name><description>[-1.2/-0.7] Abundance of [TiI/H]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[TiI/H]</name><description>[0.01/0.03] [TiI/H] internal 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[OI/FeII] uncertainty</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[NaI/FeI]L</name><description>[-0.2/1.1] LTE abundance of [NaI/FeI] (3)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[NaI/FeI]L</name><description>[0.04/0.2] [NaI/FeI]L uncertainty</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[NaI/FeI]N</name><description>[-0.08/1.1] NLTE abundance of [NaI/FeI] (3)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[NaI/FeI]N</name><description>[0.02/0.2] [NaI/FeI]N uncertainty</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[MgI/FeI]</name><description>[0.3/0.6] Abundance of [MgI/FeI]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[MgI/FeI]</name><description>[0.01/0.09] [MgI/FeI] uncertainty</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nMg</name><description>[2/3] Number of MgI lines used</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[AlI/FeI]</name><description>[0.1/1.2] Abundance of [AlI/FeI]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[AlI/FeI]</name><description>[0/0.07] [AlI/FeI] uncertainty</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nAl</name><description>[1/2] Number of AlI lines used</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[TiI/FeI]</name><description>[0.06/0.4] Abundance of [TiI/FeI]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[TiI/FeI]</name><description>[0.01/0.04] [TiI/FeI] uncertainty</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[TiII/FeII]</name><description>[0.05/0.3] Abundance of [TiII/FeII]</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[TiII/FeII]</name><description>[0.03/0.08] [TiII/FeII] uncertainty</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/813/97/table2</name><description>Wavelength, element, oscillator strength, excitation potential, and reference source of adopted lines</description><column><name>Ion</name><description>Ion identifier</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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