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<ri:Resource created="2024-04-18T18:34:33Z" 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>NH3 Observations of Cygnus X</title><shortName>J/A+A/684/A142</shortName><identifier>ivo://CDS.VizieR/J/A+A/684/A142</identifier><altIdentifier>doi:10.26093/cds/vizier.36840142</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang X.</name></creator><creator><name>Qiu K.</name></creator><creator><name>Zhang Q.</name></creator><creator><name>Cao Y.</name></creator><creator><name>Cheng Y.</name></creator><creator><name>Liu J.</name></creator><creator><name>Wang Y.</name></creator><creator><name>Lu X.</name></creator><creator><name>Pan X.</name></creator><date role="Updated">2024-11-07T20:02:23Z</date><date role="Created">2024-04-18T18:34:33Z</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>molecular-clouds</subject><subject>galaxy-kinematics</subject><subject>radio-astronomy</subject><description>The physical properties, evolution, and fragmentation of massive dense cores (MDCs, ~0.1pc) are fundamental to the understanding of high-mass star formation. We aim at characterizing the temperature, velocity dispersion, and fragmentation of the MDCs in the Cygnus X giant molecular cloud and to investigate their stability and dynamics. We present the Karl G. Jansky Very Large Array (VLA) observations of the NH_3_ (J, K) = (1,1) and (2,2) inversion lines towards 35 MDCs in Cygnus X, from which the temperature and velocity dispersion are calculated. We extract 202 fragments (~0.02pc) from the NH_3_ (1,1) moment-0 maps with the GAUSSCLUMPS algorithm. The stability of the MDCs and their NH_3_ fragments is analyzed through evaluating the corresponding kinetic, gravitational potential, and magnetic energies and the virial parameters. The MDCs in Cygnus X have a typical mean kinetic temperature TK of ~20K. Virial analysis shows that many MDCs are at sub-virialized states, indicating that the kinetic energy is insufficient to support these MDCs against their gravity. The calculated non-thermal velocity dispersions of most MDCs are at transonic to mildly supersonic levels, and the bulk motions only have a minor contribution to the velocity dispersion. As for the NH_3_ fragments, with TK~19K, their non-thermal velocity dispersions are mostly trans- to sub-sonic. Unless there is a strong magnetic field, most NH_3_ fragments are probably not at virialized states. We also find that most of the NH_3_ fragments are dynamically quiescent while only a few are active due to star formation activity.</description><source format="bibcode">2024A&amp;A...684A.142Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/684/A142</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/A+A/241/551">J/A+A/241/551 : Radio continuum in Cygnus X region (Wendker+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/375/539">J/A+A/375/539 : JHK photometry of compact HII regions in Cyg X</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/407/1039">J/A+A/407/1039 : X-ray power spectra of Cygnus X-1 (Pottschmidt+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/452/975">J/A+A/452/975 : Temporal variability of Cygnus X-1 (Axelsson+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/476/1243">J/A+A/476/1243 : Millimeter continuum mapping of Cygnus X (Motte+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A135">J/A+A/527/A135 : Gas dynamics in Massive Dense Cores in Cygnus-X</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/679">J/ApJ/720/679 : Optical spectroscopy in Cygnus X region (Beerer+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/727/114">J/ApJ/727/114 : BLAST 2005: a 10deg^2^ survey in Cygnus X (Roy+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/570/A1">J/A+A/570/A1 : Cygnus-X CO and SiO outflows datacubes</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/148/11">J/AJ/148/11 : Infrared photometry in Cygnus-X (Kryukova+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/458/3027">J/MNRAS/458/3027 : Young and embedded clusters in Cygnus-X (Maia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/883/156">J/ApJ/883/156 : Nobeyama 45m Cygnus-X CO. 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