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<ri:Resource created="2013-01-24T14:39:41Z" 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>Search for companions around nearby massive stars</title><shortName>J/ApJ/736/89</shortName><identifier>ivo://CDS.VizieR/J/ApJ/736/89</identifier><altIdentifier>doi:10.26093/cds/vizier.17360089</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Janson M.</name></creator><creator><name>Bonavita M.</name></creator><creator><name>Klahr H.</name></creator><creator><name>Lafreniere D.</name></creator><creator><name>Jayawardhana R.,Zinnecker H.</name></creator><date role="Updated">2017-12-22T05:33:26Z</date><date role="Created">2013-01-24T14:39:41Z</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>multiple-stars</subject><description>In this study, we present high-contrast imaging of 18 nearby massive stars of which 15 are in the B2-A0 spectral-type range and provide excellent sensitivity to wide companions. By comparing our sensitivities to model predictions of disk instability based on physical criteria for fragmentation and cooling, and using Monte Carlo simulations for orbital distributions, we find that ~85% of such companions should have been detected in our images on average. Given this high degree of completeness, stringent statistical limits can be set from the null-detection result, even with the limited sample size. We find that &lt;30% of massive stars form and retain disk instability planets, brown dwarfs, and very low mass stars of &lt;100M_jup_ within 300AU, at 99% confidence. These results, combined with previous findings in the literature, lead to the conclusion that core accretion is likely the dominant mode of planet formation.</description><source format="bibcode">2011ApJ...736...89J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/736/89</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/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/352/555">J/A+A/352/555 : Fundamental parameters of stars (Allende Prieto+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2048">J/AJ/126/2048 : NStars project: the Northern Sample. 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(Gray+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/152/251">J/ApJS/152/251 : Indo-US library of coude feed stellar spectra (Valdes+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/670/1367">J/ApJ/670/1367 : Gemini Deep Planet Survey (Lafreniere+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/506/501">J/A+A/506/501 : Eclipsing binaries in CoRoT-LRc01 field (Cabrera+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A52">J/A+A/509/A52 : Search for companions with VLT/NACO (Chauvin+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/525/A71">J/A+A/525/A71 : Atmospheric parameters for 1273 stars (Wu+, 2011)</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/736/89</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/736/89</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/736/89</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/736/89</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/736/89</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/736/89</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/736/89/table2 (Target stars properties)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/736/89/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/736/89/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/736/89/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>2.0969167</ra><dec>29.0904444</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/826 1704 6206 6705 9310 14906 20322 21788 23007 24480 25016 25973 27322 27574 28559 30229 30543 44903</spatial><spectral>1.1166583743361574e-19 1.2918781580533825e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/736/89?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/736/89/table2</name><description>Target stars properties</description><column><name>Name</name><description>Target name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>HIP</name><description>[677/97649] HIP number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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