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<ri:Resource created="2018-11-05T15:59:45Z" 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>Brightest cluster galaxies bright in 22um (W4BCGs)</title><shortName>J/ApJ/853/47</shortName><identifier>ivo://CDS.VizieR/J/ApJ/853/47</identifier><altIdentifier>doi:10.26093/cds/vizier.18530047</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Runge J.</name></creator><creator><name>Yan H.</name></creator><date role="Updated">2018-11-30T12:31:23Z</date><date role="Created">2018-11-05T15:59:45Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>infrared-photometry</subject><subject>redshifted</subject><subject>active-galactic-nuclei</subject><description>Brightest cluster galaxies (BCGs) are believed to have assembled most of their stars early in time and therefore should be passively evolving at low redshifts and appear "red-and-dead." However, there have been reports that a minority of low-redshift BCGs still have ongoing star formation rates (SFRs) of a few to even ~100M_{sun}_/yr. Such BCGs are found in "cool-core" ("CC") clusters, and their star formation is thought to be fueled by "cooling flow." To further investigate the implications of low-redshift, star-forming BCGs, we perform a systematic search using the 22{mu}m data ("W4" band) from the Wide-field Infrared Survey Explorer (WISE) on the GMBCG catalog, which contains 55424 BCGs at 0.1&lt;~z&lt;~0.55 identified in the Sloan Digital Sky Survey (SDSS). Our sample consists of 389 BCGs that are bright in W4 ("W4BCGs"), most being brighter than 5mJy. While some (&lt;~20%) might host active galactic nuclei, most W4BCGs should owe their strong mid-IR emissions to dust-enshrouded star formation. Their median total IR luminosity (L_IR_) is 5x10^11^L_{sun}_ (SFR~50M_{sun}_/yr), and 27% of the whole sample has L_IR_&gt;10^12^L_{sun}_ (SFR&gt;100M_{sun}_/yr). Using 10 W4BCGs that have Chandra X-ray data, we show that 7 of them are possibly in CC clusters. However, in most cases (five out of seven) the mass deposition rate cannot account for the observed SFR. This casts doubt on the idea that cooling flows are the cause of the star formation in non-quiescent BCGs.</description><source format="bibcode">2018ApJ...853...47R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/853/47</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/76">VIII/76 : Leiden/Argentine/Bonn (LAB) Survey of Galactic HI (Kalberla+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/95">VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/191/254">J/ApJS/191/254 : GMBCG galaxy cluster catalog from SDSS DR7 (Hao+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A119">J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/772/26">J/ApJ/772/26 : AGN with WISE. II. The NDWFS Bootes field (Assef+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/785/104">J/ApJ/785/104 : redMaPPer. I. Algorithm applied to SDSS DR8 (Rykoff+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/22">J/ApJS/210/22 : Herschel Stripe 82 survey (HerS) first catalog (Viero+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/L63">J/MNRAS/444/L63 : SFRs of Brightest Cluster Galaxies (Fraser-McKelvie+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/811/58">J/ApJ/811/58 : FIR properties of SDSS 0.1&lt;z&lt;5 quasars (Ma+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/462/3146">J/MNRAS/462/3146 : Herschel-ATLAS DR1 (Valiante+, 2016)</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/853/47</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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