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<ri:Resource created="2022-02-15T12:50:11Z" 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>BL Lac objects and radio galaxies comparison</title><shortName>J/ApJ/900/L34</shortName><identifier>ivo://CDS.VizieR/J/ApJ/900/L34</identifier><altIdentifier>doi:10.26093/cds/vizier.19009034</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Massaro F.</name></creator><creator><name>Capetti A.</name></creator><creator><name>Paggi A.</name></creator><creator><name>Baldi R.D.</name></creator><creator><name>Tramacere A.</name></creator><creator><name>Pillitteri I.,Campana R.</name></creator><date role="Updated">2022-05-18T13:12:10Z</date><date role="Created">2022-02-15T12:50:11Z</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>bl-lacertae-objects</subject><subject>radio-galaxies</subject><subject>redshifted</subject><subject>active-galactic-nuclei</subject><description>The most elusive and extreme subclass of active galactic nuclei (AGNs), known as BL Lac objects, shows features that can only be explained as the result of relativistic effects occurring in jets pointing at a small angle with respect to the line of sight. A longstanding issue is the identification of the BL Lac parent population with jets oriented at larger angles. According to the "unification scenario" of AGNs, radio galaxies with low luminosity and an edge-darkened radio morphology are the most promising candidate parent population of BL Lacs. Here we compare the large-scale environment, an orientation-independent property, of well-defined samples of BL Lacs with samples of radio galaxies all lying in the local universe. Our study reveals that BL Lacs and radio galaxies live in significantly different environments, challenging predictions of the unification scenario. We propose a solution to this problem proving that large-scale environments of BL Lacs are statistically consistent with those of compact radio sources, known as FR 0s, and share similar properties. This implies that highly relativistic jets are ubiquitous and are the natural outcome of the accretion of gas into the deep gravitational potential well produced by supermassive black holes.</description><source format="bibcode">2020ApJ...900L..34M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/900/L34</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/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/274">VII/274 : The Roma BZCAT - 5th edition (Massaro+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/92">VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 (Helfand+ 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/167/1">J/ApJS/167/1 : Galaxy groups and clusters from SDSS (Berlind+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/171/61">J/ApJS/171/61 : All-Sky Survey of Flat-Spectrum Radio Sources (Healey+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/752/61">J/ApJ/752/61 : Blazars in unidentified {gamma}-ray sources (Massaro+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/68">J/ApJ/748/68 : WISE IR colors of gamma-ray blazars (D'Abrusco+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/752/61">J/ApJ/752/61 : Blazars in unidentified {gamma}-ray sources (Massaro+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/120">J/AJ/146/120 : MOJAVE. X. Parsec-scale kinematics of AGNs (Lister+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/442/1693">J/MNRAS/442/1693 : Gamma-ray-loud blazars opt. polarization (Pavlidou+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/598/A49">J/A+A/598/A49 : FRICAT. FIRST cat. of FR I radio galaxies (Capetti+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/601/A81">J/A+A/601/A81 : FIRST catalog of FR II radio galaxies (Capetti+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/609/A1">J/A+A/609/A1 : FR0CAT. a FIRST cat. of FR 0 radio galaxies (Baldi+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/878/11">J/ApJ/878/11 : Type 1 vs 2 X-ray-selected COSMOS AGNs &amp; env. (Zou+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/33">J/ApJS/247/33 : Fermi LAT fourth source catalog (4FGL) (Abdollahi+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/71">J/ApJS/247/71 : Large-scale environment of radio gal. II. 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