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<ri:Resource created="2010-10-07T14:04:45Z" status="active" updated="2026-03-17T20:08:14Z" 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>Wide southern double stars</title><shortName>J/other/PASA/24.</shortName><identifier>ivo://CDS.VizieR/J/other/PASA/24.118</identifier><altIdentifier>doi:10.26093/cds/vizier/ds/cekbbi</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bauer C.</name></creator><creator><name>White G.L.</name></creator><creator><name>Blank D.</name></creator><creator><name>Jones P.A.</name></creator><date role="Updated">2026-03-17T20:08:14Z</date><date role="Created">2010-10-07T14:04:45Z</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>multiple-stars</subject><subject>visible-astronomy</subject><subject>kron-cousins-photometry</subject><description>Astrometric CCD observations have been made of wide (~3 to 60 arcsec) southern double stars selected from the Washington Double Star catalogue (WDS). Southern double stars have not been well studied in the past; typically they had not been measured since about 1930, and ~50% of them have been observed only once before our observations. Of the pairs measured ~80% show no evidence of motion since the last observation. This is Paper II in which we present the observations of 290 WDS stars in the approximate RA range 17h13m to 07h30m and in the declination range -70{deg} to -60{deg}. We suggest 412 companions for these 290 stars and list 29 (10%) pairs that have shown significant motion.</description><source format="bibcode">2007PASA...24..118B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/PASA/24.118</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/B/wds">B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/274">I/274 : CCDM (Catalog of Components of Double and Multiple 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Difference in magnitude between the primary and the secondary star in R band</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dImag</name><description>? Difference in magnitude between the primary and the secondary star in I band</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Note</name><description>[*] Note (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Prob</name><description>? 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