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<ri:Resource created="2006-02-09T07:31:00Z" status="active" updated="2025-06-13T15:25:00Z" 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>Bar-induced strengths in spiral galaxies</title><shortName>J/MNRAS/355/1251</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/355/1251</identifier><altIdentifier>doi:10.26093/cds/vizier.73551251</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Laurikainen E.</name></creator><creator><name>Salo H.</name></creator><creator><name>Buta R.</name></creator><creator><name>Vasylyev S.</name></creator><date role="Updated">2024-06-30T20:16:43Z</date><date role="Created">2006-02-09T07:31:00Z</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>galaxies</subject><subject>galaxy-classification-systems</subject><description>Bar-induced perturbation strengths are calculated for a well-defined magnitude-limited sample of 180 spiral galaxies, based on the Ohio State University Bright Galaxy Survey. 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