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<ri:Resource created="2015-08-27T07:36:53Z" 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. I.</title><shortName>J/ApJ/787/107</shortName><identifier>ivo://CDS.VizieR/J/ApJ/787/107</identifier><altIdentifier>doi:10.26093/cds/vizier.17870107</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>Baddeley A.J.</name></creator><creator><name>Broos P.S.,Sills A.</name></creator><creator><name>Bate M.R.</name></creator><creator><name>Povich M.S.</name></creator><creator><name>Luhman K.L.</name></creator><creator><name>Busk H.A.</name></creator><creator><name>Naylor T.,King R.R.</name></creator><date role="Updated">2018-02-02T10:34:12Z</date><date role="Created">2015-08-27T07:36:53Z</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>h-ii-regions</subject><subject>molecular-clouds</subject><subject>infrared-sources</subject><subject>x-ray-sources</subject><description>The clusters of young stars in massive star-forming regions show a wide range of sizes, morphologies, and numbers of stars. Their highly subclustered structures are revealed by the MYStIX project's sample of 31754 young stars in nearby sites of star formation (regions at distances &lt;3.6kpc that contain at least one O-type star.) In 17 of the regions surveyed by MYStIX, we identify subclusters of young stars using finite mixture models --collections of isothermal ellipsoids that model individual subclusters. Maximum likelihood estimation is used to estimate the model parameters, and the Akaike Information Criterion is used to determine the number of subclusters. This procedure often successfully finds famous subclusters, such as the BN/KL complex behind the Orion Nebula Cluster and the KW-object complex in M17. A catalog of 142 subclusters is presented, with 1-20 subclusters per region. The subcluster core radius distribution for this sample is peaked at 0.17pc with a standard deviation of 0.43dex, and subcluster core radius is negatively correlated with gas/dust absorption of the stars --a possible age effect. Based on the morphological arrangements of subclusters, we identify four classes of spatial structure: long chains of subclusters, clumpy structures, isolated clusters with a core-halo structure, and isolated clusters well fit by a single isothermal ellipsoid.</description><source format="bibcode">2014ApJ...787..107K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/787/107</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/ApJ/802/60">J/ApJ/802/60 : Structure or 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>Reg</name><description>Massive star-forming region (MSFR) name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Dist</name><description>[0.4/3.6] Distance to region used in MYStIX analysis (Feigelson et al. 2013ApJS..209...26F)</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logFX</name><description>[-6.8/-5.9] Apparent 0.5-8.0keV X-ray photon flux limit imposed for spatial uniformity</description><unit>ph.s**-1.cm**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ns</name><description>[246/2790] Total number of stars used in analysis</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nsp</name><description>[38/96] Percentage of all MPCMs</description><unit>%</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nx</name><description>[174/2043] Number of X-ray stars</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nir</name><description>[49/815] Number of MYStIX InfraRed Excess (MIRES) stars</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nob</name><description>[1/134] Number of OB stars</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MSFR</name><description>MYStIX region name as in tables 2 and 3; column added by CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType><flag>primary</flag></column><column><name>Nc</name><description>Number of subcluster(s) in this region</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/787/107/table2</name><description>MYStIX subcluster properties</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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 assignment (G1)</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Hour of right ascension (J2000) (1)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of declination (J2000) (1)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>amaj</name><description>[0.01/10.2] Semimajor axis of the ellipsoid core region</description><unit>pc</unit><ucd>phys.size</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>bmin</name><description>[0.01/2.1] Semiminor axis of the ellipsoid core region</description><unit>pc</unit><ucd>phys.size</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ell</name><description>[0/0.9] Ellipticity</description><ucd>src.ellipticity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA</name><description>[0/248] Orientation angle of the ellipse; east from north</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ns</name><description>[2/834] Number of stars (2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>J-H</name><description>[0.6/3] J-H color index as measure of absorption</description><unit>mag</unit><ucd>phot.color;em.IR.J;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Emed</name><description>[1/4.4] Median X-ray median energy as a measure of absorption</description><unit>keV</unit><ucd>phys.absorption;em.X-ray;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nm</name><description>Number of members in this subcluster</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>PapII</name><description>Display data from Paper II (Kuhn+, 2015, J/ApJ/802/60) for this subcluster</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>