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<ri:Resource created="2017-10-09T14:06:58Z" 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>Spatial structure of young stellar clusters. III.</title><shortName>J/ApJ/812/131</shortName><identifier>ivo://CDS.VizieR/J/ApJ/812/131</identifier><altIdentifier>doi:10.26093/cds/vizier.18120131</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kuhn M.A.</name></creator><creator><name>Feigelson E.D.</name></creator><creator><name>Getman K.V.</name></creator><creator><name>Sills A.</name></creator><creator><name>Bate M.R.</name></creator><creator><name>Borissova J.</name></creator><date role="Updated">2017-10-16T07:45:38Z</date><date role="Created">2017-10-09T14:06:58Z</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>stellar-associations</subject><subject>open-star-clusters</subject><subject>h-ii-regions</subject><description>We analyze the physical properties of stellar clusters that are detected in massive star-forming regions in the MYStIX project - a comparative, multiwavelength study of young stellar clusters within 3.6 kpc that contain at least one O-type star. Tabulated properties of subclusters in these regions include physical sizes and shapes, intrinsic numbers of stars, absorptions by the molecular clouds, and median subcluster ages. Physical signs of dynamical evolution are present in the relations of these properties, including statistically significant correlations between subcluster size, central density, and age, which are likely the result of cluster expansion after gas removal. We argue that many of the subclusters identified in Paper I (Kuhn et al. 2014, J/ApJ/787/107) are gravitationally bound because their radii are significantly less than what would be expected from freely expanding clumps of stars with a typical initial stellar velocity dispersion of ~3 km/s for star-forming regions. We explore a model for cluster formation in which structurally simpler clusters are built up hierarchically through the mergers of subclusters - subcluster mergers are indicated by an inverse relation between the numbers of stars in a subcluster and their central densities (also seen as a density versus radius relation that is less steep than would be expected from pure expansion). We discuss implications of these effects for the dynamical relaxation of young stellar clusters.</description><source format="bibcode">2015ApJ...812..131K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/812/131</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/138/227">J/AJ/138/227 : Stellar clusters in NGC 6334 complex (Feigelson+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/725/2485">J/ApJ/725/2485 : X-rays from the star-forming complex W40 (Kuhn+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/2">J/ApJS/194/2 : Chandra Carina Complex Project (CCCP) catalog (Broos+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/9">J/ApJS/194/9 : X-ray star clusters in the Carina complex (Feigelson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/192">J/AJ/144/192 : Spitzer survey of Orion A &amp; B. I. YSO catalog (Megeath+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/787/107">J/ApJ/787/107 : Spatial structure of young stellar clusters. I. (Kuhn+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/1">J/ApJS/213/1 : The MSFRs Omnibus X-ray Catalog (MOXC) (Townsley+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/27">J/ApJS/209/27 : MYStIX: the Chandra X-ray sources (Kuhn+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/28">J/ApJS/209/28 : MYStIX Wide-Field NIR data: crowded fields (King+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/29">J/ApJS/209/29 : MYStIX: Mid-IR observations and catalogs (Kuhn+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/30">J/ApJS/209/30 : MYStIX project: Bayesian matching (Naylor+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/31">J/ApJS/209/31 : The MYStIX IR-Excess Source catalog (MIRES) (Povich+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/32">J/ApJS/209/32 : Probable young stars in the MYStIX project (Broos+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/802/60">J/ApJ/802/60 : Structure of young stellar clusters. II. 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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>MSFR</name><description>MYStIX region name</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>m_MSFR</name><description>Subcluster designation as in Paper I (Kuhn+, 2014, J/ApJ/787/107) (G1)</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Class</name><description>Morphological classification</description><ucd>src.morph</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>logr4</name><description>Log of fiducial subcluster radius (=4r_c_)</description><unit>log(pc)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_logN4</name><description>[&gt;] Limit flag on logN4</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logN4</name><description>? 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