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<ri:Resource created="2013-07-12T14:43:13Z" 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>Surface brightness profiles of 10 globulars of M31</title><shortName>J/AJ/143/132</shortName><identifier>ivo://CDS.VizieR/J/AJ/143/132</identifier><altIdentifier>doi:10.26093/cds/vizier.51430132</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang S.</name></creator><creator><name>Ma J.</name></creator><date role="Updated">2017-11-10T11:15:08Z</date><date role="Created">2013-07-12T14:43:13Z</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>globular-star-clusters</subject><subject>surface-photometry</subject><description>In this paper, we present internal surface brightness profiles, using images in the F606W and F814W filter bands observed with the Advanced Camera for Surveys on the Hubble Space Telescope, for 10 globular clusters (GCs) in the outer halo of M31. Standard King models are fitted to the profiles to derive their structural and dynamical parameters. The results show that, in general, the properties of clusters in M31 and the Milky Way fall in the same regions of parameter spaces. The outer halo GCs of M31 have larger ellipticities than most of the GCs in M31 and the Milky Way. Their large ellipticities may be due to galaxy tides coming from satellite dwarf galaxies of M31 or may be related to the apparently more vigorous accretion or merger history that M31 has experienced. The tight correlation of cluster binding energy E_b_ with mass M_mod_indicates that the "fundamental plane" does exist for clusters, regardless of their host environments, which is consistent with previous studies.</description><source format="bibcode">2012AJ....143..132W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/143/132</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/A+A/544/A155">J/A+A/544/A155 : M31 globular clusters (Federici+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/531/A155">J/A+A/531/A155 : HST photometry in six M31 globular clusters (Perina+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/1043">J/AJ/140/1043 : GCs in M31 and the Galaxy (van den Bergh+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/508/1285">J/A+A/508/1285 : Metallicity estimates of M31 GCs (Galleti+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/507/1375">J/A+A/507/1375 : HST/ACS VI data of M31 globular clusters (Perina+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/770">J/AJ/138/770 : HST/WFPC survey of M31 bright young clusters (Hodge+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/94">J/AJ/137/94 : Star clusters in M31 (Caldwell+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/1667">J/AJ/138/1667 : HST survey of young clusters in M31. 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