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<ri:Resource created="2018-10-17T06:20:47Z" 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>RGB &amp; HB members of the bulge cluster NGC 6569</title><shortName>J/AJ/155/71</shortName><identifier>ivo://CDS.VizieR/J/AJ/155/71</identifier><altIdentifier>doi:10.26093/cds/vizier.51550071</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Johnson C.I.</name></creator><creator><name>Rich R.M.</name></creator><creator><name>Caldwell N.</name></creator><creator><name>Mateo M.</name></creator><creator><name>Bailey J.I.</name></creator><creator><name>Olszewski E.W.,Walker M.G.</name></creator><date role="Updated">2018-11-23T11:27:22Z</date><date role="Created">2018-10-17T06:20:47Z</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>milky-way-galaxy</subject><subject>globular-star-clusters</subject><subject>giant-stars</subject><subject>horizontal-branch-stars</subject><subject>infrared-photometry</subject><subject>radial-velocity</subject><subject>chemical-abundances</subject><subject>line-intensities</subject><description>Photometric and spectroscopic analyses have shown that the Galactic bulge cluster Terzan 5 hosts several populations with different metallicities and ages that manifest as a double red horizontal branch (HB). A recent investigation of the massive bulge cluster NGC 6569 revealed a similar, though less extended, HB luminosity split, but little is known about the cluster's detailed chemical composition. Therefore, we have used high-resolution spectra from the Magellan-M2FS and VLT-FLAMES spectrographs to investigate the chemical compositions and radial velocity distributions of red giant branch and HB stars in NGC 6569. We found the cluster to have a mean heliocentric radial velocity of -48.8 km/s ({sigma}=5.3 km/s; 148 stars) and &lt;[Fe/H]&gt;=-0.87 dex (19 stars), but the cluster's 0.05 dex [Fe/H] dispersion precludes a significant metallicity spread. NGC 6569 exhibits light- and heavy-element distributions that are common among old bulge/inner Galaxy globular clusters, including clear (anti)correlations between [O/Fe], [Na/Fe], and [Al/Fe]. The light-element data suggest that NGC 6569 may be composed of at least two distinct populations, and the cluster's low &lt;[La/Eu]&gt;=-0.11 dex indicates significant pollution with r-process material. We confirm that both HBs contain cluster members, but metallicity and light-element variations are largely ruled out as sources for the luminosity difference. However, He mass fraction differences as small as {Delta}Y~0.02 cannot be ruled out and may be sufficient to reproduce the double HB.</description><source format="bibcode">2018AJ....155...71J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/71</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/337">II/337 : VISTA Variables in the Via Lactea Survey DR1 (Saito+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/348">II/348 : VISTA Variable in the Via Lactea Survey DR2 (Minniti+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/361/272">J/MNRAS/361/272 : JHKs photometry of 4 Bulge globular clusters</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1287">J/AJ/133/1287 : JHK photometry of 24 Galactic globular clusters</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/177">J/A+A/486/177 : Bulge field stars from FLAMES-GIRAFFE spectra</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/183">J/MNRAS/383/183 : CaII triplet of RGB from VLT/FLAMES obs. (Battaglia+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/517/A81">J/A+A/517/A81 : 2nd and 3d parameters of HB of globular clusters</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/402/1729">J/MNRAS/402/1729 : JHK photometry of 36 Galactic globular clusters</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/540/A27">J/A+A/540/A27 : Spectroscopy in Galactic globular clusters (Saviane+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A76">J/A+A/563/A76 : CaII triplet equivalent widths in 30 globulars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/590/A9">J/A+A/590/A9 : RGB stars in Galactic GC stellar parameters (Dias+, 2016)</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/155/71</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/155/71</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/155/71</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/155/71</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/155/71</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/155/71</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/155/71/table2 (M2FS Star Identifiers, Coordinates, Photometry, and Velocities)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/155/71/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/155/71/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/155/71/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>273.249915</ra><dec>-31.9007</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/155/71/table3 (FLAMES Star Identifiers, Coordinates, Photometry, and Velocities)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/155/71/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/155/71/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/155/71/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>273.29745694</ra><dec>-31.80356389</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/28768 28769</spatial><spectral>7.952274030004205e-20 1.7798557115773645e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/155/71?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/155/71/table2</name><description>M2FS Star Identifiers, Coordinates, Photometry, and Velocities</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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VVV Right Ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DEdegV</name><description>? VVV Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>JmagV</name><description>[9.463/17.897]? VVV J band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>KsmagV</name><description>[8.23/17.406]? 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Uncertainty in [Mg/Fe] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Al/Fe]</name><description>[0.31/0.91] [Al/Fe] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Al/Fe]</name><description>[0.07/0.14]? Uncertainty in [Al/Fe] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Si/Fe]</name><description>[0.15/0.48] [Si/Fe] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Si/Fe]</name><description>[0.07/0.14]? Uncertainty in [Si/Fe] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ca/Fe]</name><description>[0.07/0.42] [Ca/Fe] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Ca/Fe]</name><description>[0.05/0.07]? Uncertainty in [Ca/Fe] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Cr/Fe]</name><description>[-0.27/0.3]? [Cr/Fe] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Cr/Fe]</name><description>[0.07/0.11]? Uncertainty in [Cr/Fe] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[FeI/H]</name><description>[-0.97/-0.75] [FeI/H] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeI/H]</name><description>[0.1/0.1] Uncertainty in [FeI/H] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[FeII/H]</name><description>[-0.95/-0.75] [FeII/H] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeII/H]</name><description>[0.11/0.13] Uncertainty in [FeII/H] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ni/Fe]</name><description>[-0.2/0] [Ni/Fe] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Ni/Fe]</name><description>[0.05/0.1] Uncertainty in [Ni/Fe] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[LaII/Fe]</name><description>[0.18/0.68] [LaII/Fe] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[LaII/Fe]</name><description>[0.1/0.12] Uncertainty in [LaII/Fe] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[EuII/Fe]</name><description>[0.37/0.88]? [EuII/Fe] abundance (in dex)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[EuII/Fe]</name><description>[0.09/0.12]? Uncertainty in [EuII/Fe] (in dex)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>