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<ri:Resource created="2005-03-05T16:41:22Z" 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>BV photometry of LW 55 in LMC</title><shortName>J/AJ/126/237</shortName><identifier>ivo://CDS.VizieR/J/AJ/126/237</identifier><altIdentifier>doi:10.26093/cds/vizier.51260237</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kaluzny J.</name></creator><creator><name>Rucinski S.M.</name></creator><date role="Updated">2023-04-06T16:50:58Z</date><date role="Created">2005-03-05T16:41:22Z</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>magellanic-clouds</subject><subject>open-star-clusters</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>The field of the moderately old open cluster LW 55 in the outer parts of the Large Magellanic Cloud disk was monitored for detection of short-period variable stars over two nights. Eight variables were found; all but one (a detached eclipsing binary) are small-amplitude ({Delta}V&lt;=0.1mag) pulsating stars of the {delta} Scuti, SX Phoenicis, or Doradus type. The BV color-magnitude diagram extends down to the solar-type stars at V=24 (M_V_~5.2). The cluster age is estimated at 1.5Gyr for Z=0.004 ([Fe/H]=-0.67); the surrounding stellar field is older, with an age greater than 4Gyr.</description><source format="bibcode">2003AJ....126..237K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/126/237</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/VII/183">VII/183 : Cluster System of the LMC (Kontizas+ 1990)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/117/238">J/AJ/117/238 : LMC extended catalog (Bica+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/110/533">J/A+AS/110/533 : Clusters and field stars in LMC. 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