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<ri:Resource created="2008-03-26T22:26:25Z" 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>Beta Cephei stars in the ASAS-3 data. I.</title><shortName>J/A+A/477/907</shortName><identifier>ivo://CDS.VizieR/J/A+A/477/907</identifier><altIdentifier>doi:10.26093/cds/vizier.34770907</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pigulski A.</name></creator><creator><name>Pojmanski G.</name></creator><date role="Updated">2018-01-04T08:22:30Z</date><date role="Created">2008-03-26T22:26:25Z</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><description>We analyse V-filter photometry of 41 known Beta Cephei-type stars. The ASAS-3 photometry is combined with the archival data, if available, to determine long-term stability of periods and amplitudes of excited modes. We detected amplitude changes in three Beta Cephei stars, BW Cru, V836 Cen, and V348 Nor. Period changes were found in KK Vel and V836 Cen. Our analysis shows that intrinsic period changes are more common among multiperiodic stars, apparently because they are caused by some kind of mode interaction. In addition, we found new modes for seven stars, and for ten others we provide new solutions or remove ambiguities in the detected frequencies. One candidate hybrid Beta Cephei/SPB star, HD 133823, is discovered.</description><source format="bibcode">2008A&amp;A...477..907P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/477/907</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/II/264">II/264 : ASAS Variable Stars in Southern hemisphere (Pojmanski+ 2002-05)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/477/917">J/A+A/477/917 : Beta Cephei stars in the ASAS-3 data. II. 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