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<ri:Resource created="2012-07-12T16:00:45Z" 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>COLA. III. AGN in compact IR galaxies</title><shortName>J/ApJ/720/555</shortName><identifier>ivo://CDS.VizieR/J/ApJ/720/555</identifier><altIdentifier>doi:10.26093/cds/vizier.17200555</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Parra R.</name></creator><creator><name>Conway J.E.</name></creator><creator><name>Aalto S.</name></creator><creator><name>Appleton P.N.</name></creator><creator><name>Norris R.P.,Pihlstrom Y.M.</name></creator><creator><name>Kewley L.J.</name></creator><date role="Updated">2017-06-12T08:25:08Z</date><date role="Created">2012-07-12T16:00:45Z</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>active-galactic-nuclei</subject><subject>galaxies</subject><subject>infrared-sources</subject><subject>galaxy-classification-systems</subject><subject>radio-continuum-emission</subject><description>We present results from 4.8GHz Very Large Array (VLA) and global very long baseline interferometry (VLBI) observations of the northern half of the moderate FIR luminosity (median L_IR_=10^11.01^L_{sun}_) COLA (Compact Objects in Low-power AGNs) sample of star-forming galaxies. VLBI sources are detected in a high fraction (20/90) of the galaxies observed. The radio luminosities of these cores (~10^21^W/Hz) are too large to be explained by radio supernovae or supernova remnants and we argue that they are instead powered by active galactic nuclei (AGNs). These sub-parsec scale radio cores are preferentially detected toward galaxies whose VLA maps show bright 100-500 parsec scale nuclear radio components. Since these latter structures tightly follow the FIR to radio-continuum correlation for star formation, we conclude that the AGN-powered VLBI sources are associated with compact nuclear starburst environments. The implications for possible starburst-AGN connections are discussed. The detected VLBI sources have a relatively narrow range of radio luminosity consistent with models in which intense compact Eddington-limited starbursts regulate the gas supply onto a central supermassive black hole. The high incidence of AGN radio cores in compact starbursts suggests little or no delay between the starburst phase and the onset of AGN activity.</description><source format="bibcode">2010ApJ...720..555P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/720/555</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/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/156">II/156 : IRAS Faint Source Catalog, |b| &gt; 10, Version 2.0 (Moshir+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/125">II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/1032">J/AJ/138/1032 : Filling in the gaps in the 4.85GHz sky (Healey+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/175/314">J/ApJS/175/314 : VSOP 5GHz AGN survey V. 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