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<ri:Resource created="2023-04-21T10:12:04Z" 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>C^18^O dense cores in Orion A molecular cloud</title><shortName>J/ApJS/264/35</shortName><identifier>ivo://CDS.VizieR/J/ApJS/264/35</identifier><altIdentifier>doi:10.26093/cds/vizier.22640035</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Takemura H.</name></creator><creator><name>Nakamura F.</name></creator><creator><name>Arce H.G.</name></creator><creator><name>Schneider N.</name></creator><creator><name>Ossenkopf-Okada V.,Kong S.</name></creator><creator><name>Ishii S.</name></creator><creator><name>Dobashi K.</name></creator><creator><name>Shimoikura T.</name></creator><creator><name>Sanhueza P.</name></creator><creator><name>Tsukagoshi T.,Padoan P.</name></creator><creator><name>Klessen R.S.</name></creator><creator><name>Goldsmith P.F.</name></creator><creator><name>Burkhart B.</name></creator><creator><name>Lis D.C.,Sanchez-Monge A.</name></creator><creator><name>Shimajiri Y.</name></creator><creator><name>Kawabe R.</name></creator><date role="Updated">2023-08-25T12:20:42Z</date><date role="Created">2023-04-21T10:12:04Z</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>co-line-emission</subject><subject>surveys</subject><subject>molecular-clouds</subject><subject>interstellar-medium</subject><subject>young-stellar-objects</subject><subject>stellar-masses</subject><description>The mass distribution of dense cores is a potential key to understanding the process of star formation. Applying dendrogram analysis to the CARMA-NRO Orion C^18^O (J=1-0) data, we identify 2342 dense cores, about 22% of which have virial ratios smaller than 2 and can be classified as gravitationally bound cores. The derived core mass function (CMF) for bound starless cores that are not associate with protostars has a slope similar to Salpeter's initial mass function (IMF) for the mass range above 1M_{sun}_, with a peak at ~0.1M_{sun}_. We divide the cloud into four parts based on decl., OMC-1/2/3, OMC-4/5, L1641N/V380 Ori, and L1641C, and derive the CMFs in these regions. We find that starless cores with masses greater than 10M_{sun}_ exist only in OMC-1/2/3, whereas the CMFs in OMC-4/5, L1641N, and L1641C are truncated at around 5-10M_{sun}_. From the number ratio of bound starless cores and Class II objects in each subregion, the lifetime of bound starless cores is estimated to be 5-30 freefall times, consistent with previous studies for other regions. In addition, we discuss core growth by mass accretion from the surrounding cloud material to explain the coincidence of peak masses between IMFs and CMFs. The mass accretion rate required for doubling the core mass within a core lifetime is larger than that of Bondi-Hoyle accretion by a factor of order 2. This implies that more dynamical accretion processes are required to grow cores.</description><source format="bibcode">2023ApJS..264...35T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/264/35</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/ApJ/428/693">J/ApJ/428/693 : Rosette Nebula &amp; Maddalena Cloud structures (Williams+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/123/233">J/ApJS/123/233 : Catalog of Optically selected cores (Lee+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/462/L17">J/A+A/462/L17 : Dense cores in interstellar molecular clouds (Alves+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/665/1194">J/ApJ/665/1194 : Dense cores in the Orion A cloud survey (Ikeda+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/374/1413">J/MNRAS/374/1413 : SCUBA survey of Orion (Nutter+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/181/321">J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/14">J/ApJ/748/14 : ONC population data from WFI observations (Da Rio+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/114">J/ApJ/764/114 : BVRI photometry of stars in Orion A (Hsu+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A68">J/A+A/564/A68 : Orion A GMC 13CO and C18O maps (Shimajiri+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/584/A91">J/A+A/584/A91 : Dense cores in Aquila from Herschel (Konyves+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/7">J/ApJS/217/7 : Orion A dense cores based on 1.1mm &amp; C18O (Shimajiri+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/5">J/ApJS/224/5 : Herschel Orion Protostar Survey (HOPS): SEDs (Furlan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/587/A153">J/A+A/587/A153 : VISION I. 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