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<ri:Resource created="2014-09-10T09:41:53Z" 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>Gaia-ESO Survey: NGC6705</title><shortName>J/A+A/569/A17</shortName><identifier>ivo://CDS.VizieR/J/A+A/569/A17</identifier><altIdentifier>doi:10.26093/cds/vizier.35690017</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cantat-Gaudin T.</name></creator><creator><name>Vallenari A.</name></creator><creator><name>Zaggia S.</name></creator><creator><name>Bragaglia A.</name></creator><creator><name>Sordo R.,Drew J.E.</name></creator><creator><name>Eisloeffel J.</name></creator><creator><name>Farnhill H.J.</name></creator><creator><name>Gonzalez-Solares E.</name></creator><creator><name>Greimel R.,Irwin M.J.</name></creator><creator><name>Kupcu-Yoldas A.</name></creator><creator><name>Jordi C.</name></creator><creator><name>Blomme R.</name></creator><creator><name>Sampedro L.</name></creator><creator><name>Costado M.T.,Alfaro E.</name></creator><creator><name>Smiljanic R.</name></creator><creator><name>Magrini L.</name></creator><creator><name>Donati P.</name></creator><creator><name>Friel E.D.</name></creator><creator><name>Jacobson H.,Abbas U.</name></creator><creator><name>Hatzidimitriou D.</name></creator><creator><name>Spagna A.</name></creator><creator><name>Vecchiato A.</name></creator><creator><name>Balaguer-Nunez L.,Lardo C.</name></creator><creator><name>Tosi M.</name></creator><creator><name>Pancino E.</name></creator><creator><name>Klutsch A.</name></creator><creator><name>Tautvaisiene G.</name></creator><creator><name>Drazdauskas A.,Puzeras E.</name></creator><creator><name>Jimenez-Esteban F.</name></creator><creator><name>Maiorca E.</name></creator><creator><name>Geisler D.</name></creator><creator><name>San I.,Villanova S.</name></creator><creator><name>Gilmore G.</name></creator><creator><name>Randich S.</name></creator><creator><name>Bensby T.</name></creator><creator><name>Flaccomio E.</name></creator><creator><name>Lanzafame A.,Recio-Blanco A.</name></creator><creator><name>Damiani F.</name></creator><creator><name>Hourihane A.</name></creator><creator><name>Jofre P.</name></creator><creator><name>deLaverny P.,Masseron T.</name></creator><creator><name>Morbidelli L.</name></creator><creator><name>Prisinzano L.</name></creator><creator><name>Sacco G.G.</name></creator><creator><name>Sbordone L.,Worley C.C.</name></creator><date role="Updated">2015-02-08T15:25:16Z</date><date role="Created">2014-09-10T09:41:53Z</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>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>radial-velocity</subject><description>Chemically inhomogeneous populations are observed in most globular clusters, but not in open clusters. Cluster mass seems to play a key role in the existence of multiple populations. Studying the chemical homogeneity of the most massive open clusters is needed to better understand the mechanism of their formation and determine the mass limit under which clusters cannot host multiple populations. Here we studied NGC 6705, which is a young and massive open cluster located towards the inner region of the Milky Way. This cluster is located inside the solar circle. This makes it an important tracer of the inner disk abundance gradient. This study makes use of BVI and ri photometry and comparisons with theoretical isochrones to derive the age of NGC 6705. We study the density profile of the cluster and the mass function to infer the cluster mass. Based on abundances of the chemical elements distributed in the first internal data release of the Gaia-ESO Survey, we study elemental ratios and the chemical homogeneity of the red clump stars. Radial velocities enable us to study the rotation and internal kinematics of the cluster.</description><source format="bibcode">2014A&amp;A...569A..17C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/569/A17</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/I/324">I/324 : The Initial Gaia Source List (IGSL) (Smart, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/137">VI/137 : GaiaSimu Universe Model Snapshot (Robin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/561/A94">J/A+A/561/A94 : Velocities and photometry in Trumpler 20 (Donati+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A94">J/A+A/563/A94 : Kinematics of the Gamma Vel cluster (Jeffries+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/566/A50">J/A+A/566/A50 : Classification of stellar spectra 6440-6810{AA} (Damiani+ 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/128/255">J/A+AS/128/255 : Proper motions in M 11 (Su+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/310/982">J/MNRAS/310/982 : UBVI CCD Photometry of M11 - II. (Sung+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/412/721">J/A+A/412/721 : CCD {Delta}a-photometry of 5 open clusters (Paunzen+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/119/1233">J/PASP/119/1233 : BV photometry of M11 stars (Koo+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/513/A29">J/A+A/513/A29 : RACE-OC project: M11 (NGC6705) (Messina+, 2010)</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/569/A17</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/569/A17</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/569/A17</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/569/A17</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/569/A17</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/569/A17</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/569/A17/table2 (Positions, BV photometry, radial velocities and membership probabilities)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/569/A17/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/569/A17/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/569/A17/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>282.74517</ra><dec>-6.24469</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/30215 30226</spatial><spectral>3.322582951404819e-19 4.920466254354166e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/569/A17?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/569/A17/table2</name><description>Positions, BV photometry, radial velocities and membership probabilities</description><column><name>Pmemb</name><description>[0/1] Membership probability</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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