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<ri:Resource created="2023-02-17T13:00:10Z" 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>Gaia view of Cygnus OB2 and Carina OB1 associations</title><shortName>J/MNRAS/490/440</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/490/440</identifier><altIdentifier>doi:10.26093/cds/vizier.74900440</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lim B.</name></creator><creator><name>Naze Y.</name></creator><creator><name>Gosset E.</name></creator><creator><name>Rauw G.</name></creator><date role="Updated">2024-08-20T20:14:06Z</date><date role="Created">2023-02-17T13:00:10Z</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>ob-stars</subject><subject>stellar-associations</subject><subject>stellar-spectral-types</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>proper-motions</subject><subject>astrometry</subject><description>OB associations are the prime star-forming sites in galaxies. However, the detailed formation process of such stellar systems still remains a mystery. In this context, identifying the presence of substructures may help in tracing the footprints of their formation process. Here, we present a kinematic study of the two massive OB associations Cygnus OB2 and Carina OB1 using the precise astrometry from the Gaia Data Release 2 and radial velocities. From the parallaxes of stars, these OB associations are confirmed to be genuine stellar systems. Both Cygnus OB2 and Carina OB1 are composed of a few dense clusters and a halo which have different kinematic properties: the clusters occupy regions of 5-8 parsecs in diameter and display small dispersions in proper motion, while the haloes spread over tens of parsecs with two to three times larger dispersions in proper motion. This is reminiscent of the so-called line width-size relation of molecular clouds related to turbulence. Considering that the kinematics and structural features were inherited from those of their natal clouds would then imply that the formation of OB associations may result from structure formation driven by supersonic turbulence, rather than from the dynamical evolution of individual embedded clusters.</description><source format="bibcode">2019MNRAS.490..440L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/490/440</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</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/ApJS/194/7">J/ApJS/194/7 : X-ray properties of O and B stars in Carina (Naze+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/mk">B/mk : Catalogue of Stellar Spectral Classifications</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/41">J/AJ/143/41 : UBVIc CCD photometry of star clusters Tr14 and Tr16</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/274">III/274 : Galactic O-Star Spectroscopic Survey (GOSSS) (Sota+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/603/A81">J/A+A/603/A81 : Trumpler 14 and 16 in the Carina nebula (Damiani+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/190">J/AJ/155/190 : Carina Nebula hot stars: stellar parameters and 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