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<ri:Resource created="2008-06-07T14:49:38Z" 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>Multiperiodic RR Lyrae in ASAS catalog</title><shortName>J/MNRAS/377/1263</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/377/1263</identifier><altIdentifier>doi:10.26093/cds/vizier.73771263</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Szczygiel D.M.</name></creator><creator><name>Fabrycky D.C.</name></creator><date role="Updated">2024-07-04T20:18:13Z</date><date role="Created">2008-06-07T14:49:38Z</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>variable-stars</subject><description>The All Sky Automated Survey (ASAS) monitors bright stars (8&lt;V&lt;14mag) south of declination +28{deg}. The ASAS Catalogue of Variable Stars (ACVS) presently contains 50099 objects; among them are 2212 objects classified as RR Lyrae pulsating variables. We use ASAS photometric V-band data to search for multiperiodicity in those stars. We find that 73 of 1435 RRab stars and 49 of 756 RRc stars exhibit the Blazhko effect. We observe a deficiency of RRab Blazhko variables with main pulsation periods greater than 0.65d. The Blazhko periods of RRc stars exhibit a strongly bimodal distribution. During our study we discovered the Blazhko effect with multiple periods in object ASAS 0507473351.9 = SU Col. Blazhko periods of 89.3 and 65.8d and a candidate of 29.5d were identified with periodogram peaks near the first three harmonics of the main pulsation. These observations may inspire new models of the Blazhko effect, which has eluded a consistent theory since its discovery about one hundred years ago. Long-term light curve changes were found in 29 stars. We also found 19 Galactic double mode pulsators (RRd), of which four are new discoveries, raising the number of ASAS discoveries of such objects to 16, out of 27 known in the field of our Galaxy.</description><source format="bibcode">2007MNRAS.377.1263S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/377/1263</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/J/AcA/48/35">J/AcA/48/35 : All Sky Automated Survey variable stars (Pojmamski 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/50/177">J/AcA/50/177 : All Sky Automated 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43416 43491 43580 44326 44384 44595 44600 44838 44901 45062 45086 45243 45465 45478 45704 45741 45753 45761 45767 45876 45898-45899 45957 45994 46266 46336 46441 46482 46575 46632 46792 46949 46966 46975 47074 47259 47371 47467 47510 47598 47619 47821 47867 48194 48207 48301 48363 48459 48539 48661 48715 48911</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/377/1263?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/377/1263/table2</name><description>Objects exhibiting BL1 effect (1 peak in Blazhko period range)</description><column><name>Vmag</name><description>V magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Type</name><description>Variable type</description><ucd>meta.code;src.var</ucd><dataType xsi:type="vs:VOTableType" 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