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<ri:Resource created="2021-10-22T16:58:43Z" 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>ALMA obs. of massive clouds in the CMZ</title><shortName>J/ApJ/894/L14</shortName><identifier>ivo://CDS.VizieR/J/ApJ/894/L14</identifier><altIdentifier>doi:10.26093/cds/vizier.18949014</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lu X.</name></creator><creator><name>Cheng Y.</name></creator><creator><name>Ginsburg A.</name></creator><creator><name>Longmore S.N.</name></creator><creator><name>Kruijssen J.M.D.,Battersby C.</name></creator><creator><name>Zhang Q.</name></creator><creator><name>Walker D.L.</name></creator><date role="Updated">2022-01-19T13:10:58Z</date><date role="Created">2021-10-22T16:58:43Z</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>galactic-center</subject><subject>star-forming-regions</subject><subject>molecular-clouds</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>We report Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 continuum observations of 2000au resolution toward four massive molecular clouds in the Central Molecular Zone of the Galaxy. To study gas fragmentation, we use the dendrogram method to identify cores as traced by the dust continuum emission. The four clouds exhibit different fragmentation states at the observed resolution despite having similar masses at the cloud scale (~1-5pc). Assuming a constant dust temperature of 20K, we construct core mass functions of the clouds and find a slightly top-heavy shape as compared to the canonical initial mass function, but we note several significant uncertainties that may affect this result. The characteristic spatial separation between the cores as identified by the minimum spanning tree method, ~10^4^au, and the characteristic core mass, 1-7M_{sun}_, are consistent with predictions of thermal Jeans fragmentation. The three clouds showing fragmentation may be forming OB associations (stellar mass ~10^3^M_{sun}_). None of the four clouds under investigation seem to be currently able to form massive star clusters like the Arches and the Quintuplet (&gt;~10^4^M_{sun}_), but they may form such clusters by further gas accretion onto the cores.</description><source format="bibcode">2020ApJ...894L..14L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/894/L14</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/291/943">J/A+A/291/943 : Protostellar cores (Ossenkopf+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/789/115">J/ApJ/789/115 : The Quintuplet cluster astrometry &amp; photometry (Stolte+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/853/171">J/ApJ/853/171 : mm point sources in the extended Sgr B2 cloud (Ginsburg+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/18">J/AJ/156/18 : Binary companions of evolved stars (Price-Whelan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/862/105">J/ApJ/862/105 : Core mass function across Gal. env. 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