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<ri:Resource created="2010-12-23T12:35:06Z" 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>Masses of evolved disks in PMS stars</title><shortName>J/ApJ/686/L115</shortName><identifier>ivo://CDS.VizieR/J/ApJ/686/L115</identifier><altIdentifier>doi:10.26093/cds/vizier.16869115</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cieza L.A.</name></creator><creator><name>Swift J.J.</name></creator><creator><name>Mathews G.S.</name></creator><creator><name>Williams J.P.</name></creator><date role="Updated">2017-12-22T05:33:01Z</date><date role="Created">2010-12-23T12:35:06Z</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>infrared-photometry</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><subject>pre-main-sequence-stars</subject><description>We report deep Submillimeter Array observations of 26 pre-main-sequence (PMS) stars with evolved inner disks. These observations measure the mass of the outer disk (r~20-100AU) across every stage of the dissipation of the inner disk (r&lt;10AU) as determined by the IR spectral energy distributions (SEDs). We find that only targets with high mid-IR excesses are detected and have disk masses in the 1-5M_Jup_ range, while most of our objects remain undetected to sensitivity levels of M_DISK_~0.2-1.5M_Jup_. To put these results in a more general context, we collected publicly available data to construct the optical to millimeter wavelength SEDs of over 120 additional PMS stars. We find that the near-IR and mid-IR emissions remain optically thick in objects whose disk masses span 2 orders of magnitude (~0.5-50M_Jup_). Taken together, these results imply that, in general, inner disks start to dissipate only after the outer disk has been significantly depleted of mass. This provides strong support for photoevaporation being one of the dominant processes driving disk evolution.</description><source format="bibcode">2008ApJ...686L.115C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/686/L115</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/485/155">J/A+A/485/155 : HK photometry of rho Oph PMS stars (Alves de Oliveira+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/667/308">J/ApJ/667/308 : Weak-line T Tauri in Spitzer c2d Survey. II. (Cieza+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/475/915">J/A+A/475/915 : L1489IRS observed by the submillimeter array (Brinch+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/671/1800">J/ApJ/671/1800 : SCUBA observations of {rho} Oph cloud (Andrews+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/651/L49">J/ApJ/651/L49 : Upper Sco OB association IRAC observations (Carpenter+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/452/245">J/A+A/452/245 : Near-IR photometry of PMS stars in rho Oph (Natta+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/630/381">J/ApJ/630/381 : Mid-IR imaging in {rho} Oph (Barsony+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/1040">J/AJ/121/1040 : PMS members of upper Scorpius OB association (Preibisch+,</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/686/L115</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/686/L115</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/686/L115</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/686/L115</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/686/L115</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/686/L115</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/686/L115/table1 (Submillimeter Array (SMA) sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/686/L115/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/686/L115/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/686/L115/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>55.9776292</ra><dec>32.0082861</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1539 42959 42970 42981 42983 42992 44317 44319 44321 44366 44378 44379 44389 44401</spatial><spectral>1.5174759485335645e-22 9.710690472292815e-20</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/686/L115?format=ascii</footprint><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/686/L115/table1</name><description>Submillimeter Array (SMA) sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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