<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2014-01-28T16:38:36Z" 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>Molecular clouds in the Antennae from CO(2-1)</title><shortName>J/ApJ/750/136</shortName><identifier>ivo://CDS.VizieR/J/ApJ/750/136</identifier><altIdentifier>doi:10.26093/cds/vizier.17500136</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wei L.H.</name></creator><creator><name>Keto E.</name></creator><creator><name>Ho L.C.</name></creator><date role="Updated">2014-02-13T18:39:41Z</date><date role="Created">2014-01-28T16:38:36Z</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>radio-galaxies</subject><subject>molecular-clouds</subject><subject>galaxy-kinematics</subject><subject>interstellar-medium</subject><description>Super star clusters--extremely massive clusters found predominately in starburst environments--are essential building blocks in the formation of galaxies and thought to dominate star formation in the high-redshift universe. However, the transformation from molecular gas into these ultracompact star clusters is not well understood. To study this process, we used the Submillimeter Array and the Plateau de Bure Interferometer to obtain high angular resolution (~1.5" or 160pc) images of the Antennae overlap region in CO(2-1) to search for the molecular progenitors of the super star clusters. We resolve the molecular gas distribution into a large number of clouds, extending the differential cloud mass function down to a 5{sigma} completeness limit of 3.8x10^5^M_{sun}_. We identify a distinct break in the mass function around log M_mol_/M_{sun}_{approx}6.5, which separates the molecular clouds into two distinct populations. The smaller, less massive clouds reside in more quiescent areas in the region, while the larger, more massive clouds cluster around regions of intense star formation. A broken power-law fit to the mass function yields slopes of {alpha}=-1.39+/-0.10 and {alpha}=-1.44+/-0.14 for the low- and high-mass cloud population, well matched to the mass function found for super star clusters in the Antennae galaxies. We find large velocity gradients and velocity dispersions at the locations of intense star formation, suggestive of compressive shocks. It is likely that these environmental factors contribute to the formation of the observed massive molecular clouds and super star clusters in the Antennae galaxies.</description><source format="bibcode">2012ApJ...750..136W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/750/136</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/AJ/140/75">J/AJ/140/75 : Antennae galaxies (NGC 4038/4039) revisited (Whitmore+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/948">J/ApJ/686/948 : CO in extragalactic giant molecular clouds (Bolatto+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/166/211">J/ApJS/166/211 : Chandra sources in Antennae galaxies (Zezas+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/443/41">J/A+A/443/41 : NGC 4038/4039 broad and narrow band photometry (Mengel+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/635/280">J/ApJ/635/280 : Star clusters in the Antennae galaxies (Brandl+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/660">J/AJ/127/660 : Photometry in southern tail of the Antennae (Saviane+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/599/1049">J/ApJ/599/1049 : Supergiant molecular complexes in the Antennae (Wilson+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/561/727">J/ApJ/561/727 : BVI photometry in the Antennae galaxies (Zhang+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/109/960">J/AJ/109/960 : Young star clusters in The Antennae (Whitmore+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/428/693">J/ApJ/428/693 : Rosette Nebula and Maddalena Cloud structures (Williams+ 1994)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/750/136</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/750/136</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/750/136</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/750/136</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/750/136</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/750/136</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/750/136/table2 (Cloud catalog (basic properties from clumpfind))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/750/136/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/750/136/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/750/136/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>180.47175</ra><dec>-18.8859722</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/25344</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/750/136?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/750/136/table2</name><description>Cloud catalog (basic properties from clumpfind)</description><column><name>l_logMvir</name><description>Limit flag on logMvir</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_Rad</name><description>Limit flag on Rad (1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">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>Seq</name><description>[1/132] Running sequence number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[12] Hour of right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[18] Degree of declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Vrad</name><description>[1328/1787] Velocity (V_rad_)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>[35/317] Radius in parsecs</description><unit>pc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_sigma</name><description>Limit flag on sigma (1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>sigma</name><description>[0.8/26] Velocity dispersion ({sigma}_V_)</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMmol</name><description>[4.9/8.4] Log of total molecular gas mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMvir</name><description>[4.5/8.1] Log of virial mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>