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<ri:Resource created="2016-09-26T12:21:05Z" status="active" updated="2025-06-13T15:25:00Z" 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>Abundances of NGC 6362 member stars</title><shortName>J/ApJ/824/73</shortName><identifier>ivo://CDS.VizieR/J/ApJ/824/73</identifier><altIdentifier>doi:10.26093/cds/vizier.18240073</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mucciarelli A.</name></creator><creator><name>Dalessandro E.</name></creator><creator><name>Massari D.</name></creator><creator><name>Bellazzini M.</name></creator><creator><name>Ferraro F.R.,Lanzoni B.</name></creator><creator><name>Lardo C.</name></creator><creator><name>Salaris M.</name></creator><creator><name>Cassisi S.</name></creator><date role="Updated">2017-01-23T22:00:00Z</date><date role="Created">2016-09-26T12:21:05Z</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>globular-star-clusters</subject><subject>chemical-abundances</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><description>We present the first measure of Fe and Na abundances in NGC 6362, a low-mass globular cluster (GC) where first- and second-generation stars are fully spatially mixed. A total of 160 member stars (along the red giant branch (RGB) and the red horizontal branch (RHB)) were observed with the multi-object spectrograph FLAMES at the Very Large Telescope. We find that the cluster has an iron abundance of [Fe/H]=-1.09+/-0.01dex, without evidence of intrinsic dispersion. On the other hand, the [Na/Fe] distribution turns out to be intrinsically broad and bimodal. The Na-poor and Na-rich stars populate, respectively, the bluest and the reddest RGBs detected in the color-magnitude diagrams including the U filter. The RGB is composed of a mixture of first- and second-generation stars in a similar proportion, while almost all the RHB stars belong to the first cluster generation. To date, NGC 6362 is the least massive GC where both the photometric and spectroscopic signatures of multiple populations have been detected.</description><source format="bibcode">2016ApJ...824...73M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/824/73</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/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/1995">J/MNRAS/431/1995 : Deep uVI photometry of NGC2419 (Beccari+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A41">J/A+A/549/A41 : Horizontal branch stars in 47 Tuc and M5 (Gratton+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/548/A122">J/A+A/548/A122 : Berkeley 39 stars photometry &amp; 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