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<ri:Resource created="2026-04-09T18:33:40Z" status="active" updated="2026-05-04T07:43:19Z" 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>Morphological stability of open clusters</title><shortName>J/A+A/708/A238</shortName><identifier>ivo://CDS.VizieR/J/A+A/708/A238</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li Y.</name></creator><creator><name>Hu Q.</name></creator><creator><name>Cai Y.</name></creator><creator><name>Dai Y.</name></creator><creator><name>Qin M.</name></creator><creator><name>Luo Y.</name></creator><date role="Updated">2026-05-04T07:43:19Z</date><date role="Created">2026-04-09T18:33:40Z</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>open-star-clusters</subject><subject>galaxy-classification-systems</subject><subject>visible-astronomy</subject><description>Open clusters (OCs) usually evolve gradually as the number of their members changes, which can be manifested in their morphological characteristics. Therefore, the morphological study of OCs lays the foundation for a better understanding of their formation and evolutionary processes. We aim to investigate the morphological stability of 1490 OCs and further explore the potential change of morphological stability of the OCs at different spatial positions, using the OC catalog from the literature. We delineate the two-dimensional (2D) morphology of OCs quantitatively in the projection perpendicular to the Galactic disk plane by the rose diagram and analyze the slope changes between the morphological stabilities (Score/Souter and Ncore/Nouter) and the number of members (N) within tidal radii to investigate the influence of the external environment on the OCs at different spatial positions. We define for the first time a new morphological stability parameter Ncore/Nouter, a ratio of member numbers between cluster core and outer areas within tidal radii, which has a significant positive correlation against N, with a slope of 1.140+/-0.039, significantly steeper than the 0.720+/-0.026 measured for Score/Souter . This demonstrates that the stellar density in the core is a more sensitive tracer for morphological stability than geometry. Spatially, the radial sample OCs have larger slopes of Ncore/Nouter and Score/Souter against N, with 1.083+/-0.116 and 0.733+/-0.080, respectively, whereas those in the tangential direction 1.013+/-0.110 and 0.529+/-0.075, respectively, which means that the impact on sample OCs from tidal forces directed toward the Galactic center is possibly stronger than that from the shear force caused by the differential rotation of the Galactic disk. Moreover, the sample OCs within 90{deg} of the Galactic center, closer to the bar, exhibit slopes below 0.6 of Score /Souter against N, indicating heightened external perturbations and diminished stability. But the opposite is true for the side greater than 90{deg}. Thus, this illustrates that the influence of the external environment on our sample OCs is asymmetrical. Besides, the sample OCs younger than 30Myr display a shallow slope of 0.751+/-0.166, with those older than 800Myr (1.442+/-0.128), reflecting that young OCs likely endure both internal disruptions, such as early dynamical heating weakening core binding and more severe external disturbances, compared to older OCs. The morphological stability of OCs is not only determined by their gravitational binding, but also strongly modulated by the external environment in which they are located.</description><source format="bibcode">2026A&amp;A...708A.238L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/708/A238</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></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/A+A/708/A238</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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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="14*">char</dataType></column><column><name>RA_ICRS</name><description>Right ascension (ICRS)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Rt</name><description>Mean of the tidal radius</description><unit>pc</unit><ucd>phys.size.radius;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rt</name><description>Mean of the tidal radius error</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rcore</name><description>Core radius obtained by rose diagram method</description><ucd>phys.size.radius;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rcore</name><description>Core radius obtained by rose diagram method error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N</name><description>Number of member stars within the tidal radius of each OC</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_N</name><description>Number of member stars within the tidal radius of each OC error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Score</name><description>Area within the core region of each OC, {pi}Rcore^2^</description><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Score</name><description>Area within the core region of each OC error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Souter</name><description>Area within the outer region of each OC, sum of all areas in the sectors minus the core area</description><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Souter</name><description>Area within the outer region of each OC error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ncore</name><description>Number of member stars in the core region of each OC</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ncore</name><description>Number of member stars in the core region of each OC error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nouter</name><description>Number of member stars in the outer region of each OC</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Nouter</name><description>Number of member stars in the outer region of each OC error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>