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<ri:Resource created="2008-05-27T15:22:16Z" 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>Warm dust near methanol masers</title><shortName>J/A+A/410/597</shortName><identifier>ivo://CDS.VizieR/J/A+A/410/597</identifier><altIdentifier>doi:10.26093/cds/vizier.34100597</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Walsh A.J.</name></creator><creator><name>Macdonald G.H.</name></creator><creator><name>Alvey N.D.S.</name></creator><creator><name>Burton M.G.</name></creator><creator><name>Lee J.-K.</name></creator><date role="Updated">2008-05-27T15:24:16Z</date><date role="Created">2008-05-27T15:22:16Z</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>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>infrared-sources</subject><subject>radial-velocity</subject><description>Continuum emission at 450 and 850{mu}m from warm dust has been mapped in the fields of 71 methanol masers. Within these fields lie 30 centimetre-wave radio continuum sources and an additional 13 methanol maser sites. Sub-mm emission is detected at all but one of the maser sites, confirming the association of methanol maser emission with deeply embedded objects. Measured bolometric luminosities confirm that methanol maser emission is an excellent signpost of high-mass star formation. Examples of nearby isolated maserless dust cores may be harbouring massive protostars at an earlier evolutionary stage.</description><source format="bibcode">2003A&amp;A...410..597W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/410/597</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/AZh/72/22">J/AZh/72/22 : A 95 GHz Survey of Methanol Masers (Valtts+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/110/81">J/A+AS/110/81 : Methanol masers towards IRAS sources (van der Walt+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/134/115">J/A+AS/134/115 : Medicina 6.7GHz methanol masers survey (Slysh+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/143/269">J/A+AS/143/269 : 6.7GHz methanol maser emission survey (Szymczak+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/413/233">J/A+A/413/233 : 12.2 GHz methanol survey (Blaszkiewicz+, 2004)</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/A+A/410/597</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/410/597</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/410/597</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/410/597</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/410/597</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/410/597</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/A+A/410/597/table1 (Sub-mm source characteristics)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/410/597/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/410/597/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/410/597/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>266.51625</ra><dec>-28.416111</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/28829-28831 28896 28912-28913 28918-28919 28925 29090-29092 29094 29096-29097 29100-29101 29103 29115-29116 29160 29461 29510-29511 29529 29532-29533 30218-30219 30241 30256 30259 30262 30268-30269</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/410/597?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/410/597/table1</name><description>Sub-mm source characteristics</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MolTrans</name><description>Name of the associated molecular transition to the sub-mm source</description><ucd>meta.id;phys.mol</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>RV</name><description>? Radial velocity of the associated molecular transition</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_RV</name><description>? Reference for radial velocity, in refs.dat file</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RVCH3OH</name><description>? 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