<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2022-02-02T13:48:44Z" 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>Abundances in 2 metal-poor GCs, M53 &amp; NGC5053</title><shortName>J/ApJ/900/146</shortName><identifier>ivo://CDS.VizieR/J/ApJ/900/146</identifier><altIdentifier>doi:10.26093/cds/vizier.19000146</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chun S.-H.</name></creator><creator><name>Lee J.-J.</name></creator><creator><name>Lim D.</name></creator><date role="Updated">2022-08-25T11:25:14Z</date><date role="Created">2022-02-02T13:48:44Z</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>effective-temperature</subject><subject>infrared-sources</subject><description>We search for extratidal stars around two metal-poor Galactic globular clusters, M53 and NGC 5053, using the near-infrared APOGEE spectra. Applying the t-distributed stochastic neighbor embedding (t-SNE) algorithm on the chemical abundances and radial velocities results in identification of two isolated stellar groups composed of cluster member stars in the t-SNE projection plane. With additional selection criteria of radial velocity, location in the color-magnitude diagram, and abundances from a manual chemical analysis, we find a total of 73 cluster member candidates; seven extratidal stars are found beyond the tidal radii of the two clusters. The extratidal stars around the clusters tend to be located along the leading direction of the cluster proper motion, and the individual proper motion of these stars also seems to be compatible to those of clusters. Interestingly, we find that one extratidal star of NGC 5053 is located on the southern outskirts of M53, which is part of common stellar envelope by the tidal interaction between two clusters. We discuss the nature of this star in the context of the tidal interaction between two clusters. We find apparent Mg-Al anticorrelations with a clear gap and spread (~0.9dex) in Al abundances for both clusters, and a light Si abundance spread (~0.3dex) for NGC 5053. Since all extratidal stars have Mg-enhanced and Al-depleted features, they could be first-generation stars of two globular clusters. Our results support that M53 and NGC5053 originated in dwarf galaxies and are surrounded by extended stellar substructures of more numerous populations of clusters.</description><source format="bibcode">2020ApJ...900..146C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/900/146</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/195">VII/195 : Globular Clusters in the Milky Way (Harris, 1996)</relatedResource><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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/150">V/150 : Updated cat. of variable stars in globular clusters (Clement+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/1489">J/AJ/112/1489 : Spectroscopic survey for binaries in NGC 5053 (Yan+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/320/776">J/A+A/320/776 : Tidal radii of 7 globular clusters (Lehmann+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/358/547">J/A+A/358/547 : M53 variable stars V light curves (Kopacki, 2000)</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/497/497">J/A+A/497/497 : Physical param. from JHK flux (Gonzalez-Hernandez+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/402/226">J/MNRAS/402/226 : NGC 5053 variables VrI light curves (Arellano Ferro+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/164">J/ApJ/757/164 : Oxygen abundances of dwarf stars (Ramirez+, 2012)</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/ApJ/804/109">J/ApJ/804/109 : Equivalent widths of RGB stars in NGC 5053 (Boberg+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/153">J/AJ/149/153 : Abundances of red giants in 10 GCs (Meszaros+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/808/16">J/ApJ/808/16 : Cannon: a new approach to determine abundances (Ness+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/824/5">J/ApJ/824/5 : Chemical abundances in NGC 5024 (M53) (Boberg+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for APOGEE chemical elements (Garcia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/465/501">J/MNRAS/465/501 : APOGEE N-rich stars in inner Galaxy (Schiavon+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/228/24">J/ApJS/228/24 : GALAH semi-automated classification scheme (Traven+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/865/44">J/ApJ/865/44 : Abundances of evolved stars from IGRINS. I. (Afsar+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/126">J/AJ/156/126 : Stellar abundances from BACCHUS analysis (Jonsson+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/482/5138">J/MNRAS/482/5138 : Galactic GC mean proper motions &amp; vel. (Baumgardt+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/622/A191">J/A+A/622/A191 : 885 globular cluster giants abundances (Masseron+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/484/2832">J/MNRAS/484/2832 : Proper motions of MW globular clusters (Vasiliev, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/637/A98">J/A+A/637/A98 : Globular cluster escapees in the Gal. halo (Hanke+, 2020)</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/ApJ/900/146</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/900/146</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/900/146</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/900/146</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/900/146</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/900/146</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/ApJ/900/146/table3 (Stellar parameters, metallicity, and abundances of M53 and NGC 5053)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/900/146/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/900/146/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/900/146/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>205.9514631</ra><dec>19.5190261</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/8846 8870 26606 27922 27973 27975 27981 27984 27986 27992</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/900/146?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/900/146/table3</name><description>Stellar parameters, metallicity, and abundances of M53 and NGC 5053</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>2MASS</name><description>2MASS identifier (HHMMSSss+DDMMSSs)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>Teff</name><description>[4120/5120] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[0.5/1.94] log, surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vt</name><description>[1.66/2.09] microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FeH</name><description>[-2.33/-1.8] Metallicity</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FeH</name><description>[0.006/0.14] Uncertainty in FeH</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MgFe</name><description>[0.005/0.66]? Mg/Fe relative abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MgFe</name><description>[0.014/0.14]? Uncertainty in MgFe</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AlFe</name><description>[-0.42/1.3]? Al/Fe relative abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_AlFe</name><description>[0.01/0.2]? Uncertainty in AlFe</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SiFe</name><description>[0.2/0.65]? Si/Fe relative abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_SiFe</name><description>[0.012/0.18]? Uncertainty in SiFe</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Cluster</name><description>Cluster surveyed ("M53"=44 occurrences or "NGC 5053"=21 occurrences)</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>AP</name><description>Display data from APOGEE-2 DR16 (III/284)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>N15</name><description>Display data from Ness+, 2015, J/ApJ/808/16</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>