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<ri:Resource created="2026-06-25T08:10:16Z" status="active" updated="2026-06-25T07:27:44Z" 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>3D kinematics in the ONC. II. Mass-dependent results</title><shortName>J/ApJ/962/174</shortName><identifier>ivo://CDS.VizieR/J/ApJ/962/174</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wei L.</name></creator><creator><name>Theissen C.A.</name></creator><creator><name>Konopacky Q.M.</name></creator><creator><name>Lu J.R.</name></creator><creator><name>Hsu C.-C.</name></creator><creator><name>Kim D.</name></creator><date role="Updated">2026-06-25T07:27:44Z</date><date role="Created">2026-06-25T08:10:16Z</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>star-forming-regions</subject><subject>radial-velocity</subject><subject>effective-temperature</subject><subject>proper-motions</subject><subject>stellar-masses</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><description>We present the kinematic analysis of 246 stars within 4' from the center of Orion Nebula Cluster (ONC), the closest massive star cluster with active star formation across the full mass range, which provides valuable insights in the formation and evolution of star cluster on an individual-star basis. High-precision radial velocities and surface temperatures are retrieved from spectra acquired by the NIRSPEC instrument used with adaptive optics (NIRSPAO) on the Keck II 10m telescope. A 3D kinematic map is then constructed by combining with the proper motions previously measured by the Hubble Space Telescope Advanced Camera for Surveys/WFPC2/WFC3IR and Keck II NIRC2. The measured root-mean-squared velocity dispersion is 2.26+/-0.08km/s, significantly higher than the virial equilibrium's requirement of 1.73km/s, suggesting that the ONC core is supervirial, consistent with previous findings. Energy equipartition is not detected in the cluster. Most notably, the velocity of each star relative to its neighbors is found to be negatively correlated with stellar mass. Low-mass stars moving faster than their surrounding stars in a supervirial cluster suggests that the initial masses of forming stars may be related to their initial kinematic states. Additionally, a clockwise rotation preference is detected. A weak sign of inverse mass segregation is also identified among stars excluding the Trapezium stars, although it could be a sample bias. Finally, this study reports the discovery of four new candidate spectroscopic binary systems.</description><source format="bibcode">2024ApJ...962..174W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/962/174</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/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/357">I/357 : Gaia DR3 Part 3. 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Stellar mass based on MIST model (2016ApJS..222....8D, 2016ApJ...823..102C)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ms-MIST</name><description>[0/0.7]? Uncertainty of Ms-MIST</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ms-BHAC15</name><description>[0.02/1.4]? Stellar mass based on BHAC15 model (2015A&amp;A...577A..42B)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ms-BHAC15</name><description>[0/0.21]? Uncertainty of Ms-BHAC15</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ms-Feiden</name><description>[0.1/3]? Stellar mass based on Feiden model (2016A&amp;A...593A..99F)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ms-Feiden</name><description>[0/0.7]? Uncertainty of Ms-Feiden</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ms-Palla</name><description>[0.1/2.5]? Stellar mass based on Palla model (1999ApJ...525..772P)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ms-Palla</name><description>[0/0.51]? Uncertainty of Ms-Palla</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>m_[HC2000]</name><description>Component on [HC2000]</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table><table><name>J/ApJ/962/174/table1</name><description>Log of NIRSPEC with AO system (NIRSPAO) observations</description><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>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>Results</name><description>Display the NIRSPAO forward-modeling results for this source (link to Table 3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>[HC2000]</name><description>HC2000 identifier in Hillenbrand+ 2000, J/ApJ/540/236</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>m_[HC2000]</name><description>Component letter on [HC2000]</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Date</name><description>Date of observation (UT)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Nfr</name><description>[2/6] Number of ABBA frames</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Exp</name><description>[60/1200] Exposure time per frame</description><unit>s</unit><ucd>obs.exposure;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>T22</name><description>Display the data from Theissen+ 2022, J/ApJ/926/141</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>