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<ri:Resource created="2012-04-02T13:19:13Z" 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>g'r'i' and redshift of Abell 2254 galaxies</title><shortName>J/A+A/536/A89</shortName><identifier>ivo://CDS.VizieR/J/A+A/536/A89</identifier><altIdentifier>doi:10.26093/cds/vizier.35360089</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Girardi M.</name></creator><creator><name>Bardelli S.</name></creator><creator><name>Barrena R.</name></creator><creator><name>Boschin W.</name></creator><creator><name>Gastaldello F.</name></creator><creator><name>Nonino M.</name></creator><date role="Updated">2017-12-15T10:54:48Z</date><date role="Created">2012-04-02T13:19:13Z</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>radial-velocity</subject><description>The mechanisms giving rise to diffuse radio emission in galaxy clusters and, in particular, their connection with cluster mergers are still being debated. We explore the internal dynamics of Abell 2254, which has been shown to host a very clumpy and irregular radio halo. Our analysis is mainly based on redshift data for 128 galaxies acquired at the Telescopio Nazionale Galileo. We combined galaxy velocities and positions to select 110 cluster galaxies and analyze its internal dynamics. We also used new (g', r', i') photometric data acquired at the Isaac Newton Telescope, and (V, i') photometric data available in the Subaru Archive. 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