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<ri:Resource created="2011-04-04T15:32:15Z" 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>Globular cluster in nearby dwarf galaxies. II</title><shortName>J/MNRAS/396/1075</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/396/1075</identifier><altIdentifier>doi:10.26093/cds/vizier.73961075</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Georgiev I.Y.</name></creator><creator><name>Hilker M.</name></creator><creator><name>Puzia T.H.</name></creator><creator><name>Goudfrooij P.</name></creator><creator><name>Baumgardt H.</name></creator><date role="Updated">2024-07-08T20:15:55Z</date><date role="Created">2011-04-04T15:32:15Z</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>galaxies</subject><subject>stellar-associations</subject><subject>galaxy-classification-systems</subject><description>We compare nuclear globular clusters (nGCs) in dwarf galaxies and Galactic GCs with extended (hot) horizontal branches (EHB-GCs) in order to test the suggested external origin of the latter and the conditions at which GC self-enrichment can operate. Using luminosities and structural parameters of nGCs in low-mass (mainly late-type) dwarf galaxies from Hubble Space Telescope (HST)/Advanced Camera for Surveys (ACS) imaging, we derive the present-day escape velocities (Vesc) of stellar ejecta to reach the cluster tidal radius and compare them with those of EHB-GCs.</description><source format="bibcode">2009MNRAS.396.1075G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/396/1075</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/AJ/135/1858">J/AJ/135/1858 : Old globular clusters in dwarf irr. galaxies (Georgiev+ 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/392/879">J/MNRAS/392/879 : Globular clusters in nearby dwarf galaxies (Georgiev+, 2009)</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/MNRAS/396/1075</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/396/1075</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/396/1075</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/396/1075</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><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>GType</name><description>Host galaxy type (dIrr, dE, dSph or Sm)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>[GPH2009]</name><description>Cluster name (Georgiev et al. 2009, Cat. 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Projected distance normalized to galaxy effective radius reff (rp/reff) (2)</description><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from Paper I (Georgiev et al., J/MNRAS/392/879) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column></table><table><name>J/MNRAS/396/1075/tables4</name><description>Properties of Galactic globular clusters</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>Name</name><description>Cluster name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>OName</name><description>Other name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>E(B-V)</name><description>Foreground Galactic extinction E(B-V) from Harris (1996, Cat. VII/195)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(V-I)0</name><description>? Cluster V-I color index (corrected for foreground extinction)</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VMAG</name><description>Cluster absolute V magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM</name><description>log10 of cluster mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rh</name><description>Cluster half-light radius</description><unit>pc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>c</name><description>Concentration index, c=log(rt/rc) (ratio of tidal to core radius)</description><ucd>meta.code;spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vesc</name><description>Escape velocity to reach the tidal radius</description><unit>km/s</unit><ucd>phys.veloc.escape</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Matallicity</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HBR</name><description>? 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