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<ri:Resource created="2026-01-30T10:47:10Z" status="active" updated="2026-07-02T12:00:53Z" 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>Influence of outflow feedback in ATLASGAL clumps</title><shortName>J/ApJ/956/50</shortName><identifier>ivo://CDS.VizieR/J/ApJ/956/50</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-xw-1j</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li Q.</name></creator><creator><name>Li M.</name></creator><creator><name>Zhang Li</name></creator><creator><name>Pei S.</name></creator><creator><name>Chang Z.</name></creator><creator><name>Zhang Yi</name></creator><date role="Updated">2026-07-02T12:00:53Z</date><date role="Created">2026-01-30T10:47:10Z</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>star-forming-regions</subject><subject>interstellar-medium</subject><subject>radio-sources</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>We analyzed the influence of outflow feedback from two perspectives: turbulent support and potential disruptive effect, of which 694 clumps and 188 have been identified as outflow candidates. For turbulent support, we find the slopes of E_turb_-R_clump_ (turbulent energy and radius of the clump) and P_turb_-R_clump_ (turbulent momentum and radius of the clump) have no difference and are consistent with expected values whether there is outflow feedback in clumps or not. The ratios of the outflow energy and momentum to the turbulence energy and momentum (E_flow_/E_turb_, P_flow_/P_turb_) show that the majority of clumps have not enough energy and momentum to support turbulence. Meanwhile, there is no correlation between the velocity dispersion and radius. For potential disruptive effects, we conclude that it is impossible for the outflow activities to disrupt entire clumps and as the mass of the clumps increases, the clumps becomes harder to destroy. Finally, we do not see evidence that the virial parameter changes significantly whether the clumps have outflow candidates or not.</description><source format="bibcode">2023ApJ...956...50L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/956/50</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/499/175">J/A+A/499/175 : ^12^CO(2-1) map of NGC 2264-C (Maury+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/1752">J/MNRAS/431/1752 : ATLASGAL 6.7GHz methanol masers (Urquhart+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/A94">J/A+A/557/A94 : SiO &amp; HCO+ massive molecular outflows (Sanchez-Monge+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A45">J/A+A/549/A45 : ATLASGAL Compact Source Catalog: 330&lt;l&lt;21 (Contreras+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A41">J/A+A/568/A41 : ATLASGAL Compact Source Catalog: 280&lt;l&lt;60 (Urquhart+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/566">J/MNRAS/444/566 : Methanol maser associated outflows (de Villiers+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/450/1926">J/MNRAS/450/1926 : Infall motions in massive star-forming regions (He+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/461/2288">J/MNRAS/461/2288 : Infall motions in massive star-forming regions (He+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PASA/33.30">J/other/PASA/33.30 : MALT90 Catalogue (Rathborne+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/473/1059">J/MNRAS/473/1059 : Galactic clump properties (Urquhart+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/3">J/ApJS/235/3 : Massive outflows with ATLASGAL clump data (Yang+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/477/2220">J/MNRAS/477/2220 : Larson relations in massive clumps (Traficante+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/867/167">J/ApJ/867/167 : High-mass outflows from the COHRS CO(3-2) survey (Li+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/488/4638">J/MNRAS/488/4638 : Infall &amp; outflow on massive star-forming regions (Li+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/251/26">J/ApJS/251/26 : CO outflow cand. toward W3/4/5 complex. 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