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<ri:Resource created="2021-03-17T09:06:57Z" 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>Internal kinematics of 9 globular clusters with HST</title><shortName>J/AJ/161/41</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/41</identifier><altIdentifier>doi:10.26093/cds/vizier.51610041</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cohen R.E.</name></creator><creator><name>Bellini A.</name></creator><creator><name>Libralato M.</name></creator><creator><name>Correnti M.</name></creator><creator><name>Brown T.M.</name></creator><creator><name>Kalirai J.S.</name></creator><date role="Updated">2022-09-30T21:41:34Z</date><date role="Created">2021-03-17T09:06:57Z</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>hst-photometry</subject><subject>visible-astronomy</subject><subject>proper-motions</subject><description>This study constitutes part of a larger effort aimed at better characterizing the Galactic globular clusters (GGCs) located toward the inner Milky Way bulge and disk. Here, we focus on internal kinematics of nine GGCs, obtained from space-based imaging over time baselines of &gt;9yr. We exploit multiple avenues to assess the dynamical state of the target GGCs, constructing radial profiles of projected stellar density, proper motion dispersion, and anisotropy. We posit that two-thirds (6/9) of our target GGCs are in an advanced dynamical state, and are close to (or have recently undergone) core-collapse, supported by at least two lines of evidence. First, we find relatively steep proper motion dispersion profiles, in accord with literature values for core-collapsed GGCs. Second, we find that our sample is, in the mean, isotropic even out to their half-light radii, although one of our target clusters (NGC6380) is tangentially anisotropic at &gt;1{sigma} beyond its half-light radius, in accord with theoretical predictions for clusters evolving in strong tidal fields. Our proper motion dispersion and anisotropy profiles are made publicly available.</description><source format="bibcode">2021AJ....161...41C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/41</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><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/J/AJ/109/218">J/AJ/109/218 : Catalogue of globular cluster profiles (Trager+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/161/304">J/ApJS/161/304 : Star clusters in Milky Way &amp; satellites (McLaughlin+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/447">J/AJ/132/447 : Surface Brightness 38 Gal. 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