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<ri:Resource created="2016-09-07T08:43:54Z" 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>Cygnus OB2 DANCe: Proper motion study</title><shortName>J/MNRAS/460/2593</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/460/2593</identifier><altIdentifier>doi:10.26093/cds/vizier.74602593</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wright N.J.</name></creator><creator><name>Bouy H.</name></creator><creator><name>Drew J.E.</name></creator><creator><name>Sarro L.M.</name></creator><creator><name>Bertin E.</name></creator><creator><name>Cuillandre J.-C.,Barrado D.</name></creator><date role="Updated">2024-08-16T20:17:20Z</date><date role="Created">2016-09-07T08:43:54Z</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>proper-motions</subject><description>We present a high-precision proper motion study of 873 X-ray and spectroscopically selected stars in the massive OB association Cygnus OB2 as part of the DANCe project. These were calculated from images spanning a 15-year baseline and have typical precisions &lt;1mas/yr. We calculate the velocity dispersion in the two axes to be 13.0^+0.8^_-0.7_ and 9.1^+0.5^_-0.5_km/s, using a 2-component, 2-dimensional model that takes into account the uncertainties on the measurements. This gives a 3-dimensional velocity dispersion of 17.8+/-0.6km/s implying a virial mass significantly larger than the observed stellar mass, confirming that the association is gravitationally unbound. The association appears to be dynamically unevolved, as evidenced by considerable kinematic substructure, non-isotropic velocity dispersions and a lack of energy equipartition. The proper motions show no evidence for a global expansion pattern, with approximately the same amount of kinetic energy in expansion as there is in contraction, which argues against the association being an expanded star cluster disrupted by process such as residual gas expulsion or tidal heating. The kinematic substructures, which appear to be close to virial equilibrium and have typical masses of 40-400M_{sun}_, also do not appear to have been affected by the expulsion of the residual gas. We conclude that Cyg OB2 was most likely born highly substructured and globally unbound, with the individual subgroups born in (or close to) virial equilibrium, and that the OB association has not experienced significant dynamical evolution since then.</description><source format="bibcode">2016MNRAS.460.2593W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/460/2593</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/643/238">J/ApJ/643/238 : Chandra/2MASS sources in Cygnus OB2 (Butt+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/474/495">J/A+A/474/495 : X-ray flares from Cygnus OB2 young stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/464/211">J/A+A/464/211 : Chandra and near-IR obs. of Cyg OB2 (Albacete Colombo+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/472/557">J/A+A/472/557 : Cygnus OB2 region 610MHz sources (Marti+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/453">J/A+A/486/453 : NIR photometry of early-type stars in Cyg OB2 (Comeron+ 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/84">J/ApJS/184/84 : X-ray sources in Cyg OB2 region (Wright+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/543/A101">J/A+A/543/A101 : OB stars in Cygnus OB2 association (Comeron+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/713/871">J/ApJ/713/871 : Sources in star-forming region Cyg-OB2 from X-ray</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/449/741">J/MNRAS/449/741 : The massive star population of Cygnus OB2 (Wright+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/575/A120">J/A+A/575/A120 : DANCe study of M35 (NGC 2168) (Bouy+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/577/A148">J/A+A/577/A148 : The Seven Sisters DANCe. 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