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<ri:Resource created="2022-11-08T06:44:05Z" 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>Gaia structural parameters of 256 open clusters</title><shortName>J/AJ/164/54</shortName><identifier>ivo://CDS.VizieR/J/AJ/164/54</identifier><altIdentifier>doi:10.26093/cds/vizier.51640054</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhong J.</name></creator><creator><name>Chen Li</name></creator><creator><name>Jiang Y.</name></creator><creator><name>Qin S.</name></creator><creator><name>Hou J.</name></creator><date role="Updated">2023-01-24T12:47:54Z</date><date role="Created">2022-11-08T06:44:05Z</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>open-star-clusters</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>proper-motions</subject><description>With the help of Gaia data, it is noted that in addition to the core components, there are low-density outer halo components in the extended region of open clusters. In order to study the extended structure beyond the core radius of the cluster (~10pc), based on Gaia Early Data Release 3, taking up to 50pc as the searching radius, we use the pyUPMASK algorithm to redetermine the member stars of the open cluster within 1-2kpc. We obtain the member stars of 256 open clusters, especially those located in the outer halo region of open clusters. Furthermore, we find that the radial density profile in the outer region for most open clusters deviates from the Kings profile. In order to better describe the internal and external structural characteristics of open clusters, we propose a two-component model: a core component with a King model distribution and an outer halo component with a logarithmic Gaussian distribution, and then suggest using four radii (rc, rt, ro, re) for describing the structure and distribution profile of star clusters, where rt and re represent the boundaries of the core component and outer halo component, respectively. Finally, we provide a catalog of 256 clusters with structural parameters. In addition, our study shows the sizes of these radii are statistically linearly related, which indicates that the inner and outer regions of the cluster are interrelated and follow similar evolutionary processes. Further, we show that the structure of two components can be used to better trace the cluster evolution properties at different stages.</description><source format="bibcode">2022AJ....164...54Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/164/54</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/B/ocl">B/ocl : Optically visible open clusters and Candidates (Dias+ 2002-2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/543/A156">J/A+A/543/A156 : Milky Way global survey of star clusters (Kharchenko+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A53">J/A+A/558/A53 : Milky Way global survey star clusters. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster name in CG20 (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>RA_ICRS</name><description>[0.5/354] Mean right ascension of members in CG20, (ICRS) at Ep=2015.5 (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>[-71/86] Mean declination of members in CG20, (ICRS) at Ep=2015.5 (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>pmRA</name><description>[-11.4/7.68] Mean proper motion along RA of members in CG20, pmRA*cosDE (1)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>[-9.74/12] Mean proper motion along DE of members in CG20 (1)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>[0.44/1.06] Mean parallax members in CG20 (1)</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[1003/1992] Most likely distance of clusters in CG20 (1)</description><unit>pc</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>Age</name><description>[7.0/9.85] Estimated cluster age in CG20 (1)</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>KDE</name><description>[0.271/0.589] Bandwidth of kernel density estimation</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Angh</name><description>[0.03/2.31] Angular size of half number radius</description><unit>deg</unit><ucd>meta.number;phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Angc</name><description>[0.06/2.3] Angular size of King's core radius derived by the core members</description><unit>deg</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Angc</name><description>[0.001/3] Measurement uncertainty of Angc</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Angt</name><description>[0.11/6.9] Angular size of King's tidal radius derived by the core members</description><unit>deg</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Angt</name><description>[0.003/9] Measurement uncertainty of Angt</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ango</name><description>[0.09/2.63]? Angular size of mean radius of outer halo members</description><unit>deg</unit><ucd>phys.angSize;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ango</name><description>[0/0.13]? Measurement uncertainty of Ango</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ange</name><description>[0.19/7.43]? Angular size of boundary radius of outer halo members</description><unit>deg</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ange</name><description>[0.003/2]? Measurement uncertainty of Ange</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Radh</name><description>[1.3/58] Physical size of half number radius</description><unit>pc</unit><ucd>meta.number;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Radc</name><description>[2.1/54.5] Physical size of King's core radius derived by the core members</description><unit>pc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Radt</name><description>[3.6/214] Physical size of King's tidal radius derived by the core members</description><unit>pc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rado</name><description>[2.8/61.2]? 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