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<ri:Resource created="2015-10-29T08:06:45Z" 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>Speckle-interferometry in Melotte 111</title><shortName>J/AJ/150/16</shortName><identifier>ivo://CDS.VizieR/J/AJ/150/16</identifier><altIdentifier>doi:10.26093/cds/vizier.51500016</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Guerrero C.A.</name></creator><creator><name>Orlov V.G.</name></creator><creator><name>Monroy-Rodriguez M.A.</name></creator><creator><name>Borges Fernandes M.</name></creator><date role="Updated">2018-01-05T08:56:06Z</date><date role="Created">2015-10-29T08:06:45Z</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>open-star-clusters</subject><subject>interferometry</subject><subject>multiple-stars</subject><subject>astronomical-object-identification</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>We present a high-angular resolution survey for the search of binary and multiple stars in the Galactic open cluster Melotte 111. Combining our own speckle-interferometric observations with data taken from the literature, we found a ratio of the number of single to multiple stars to be 29:8:0:0:0:1 for the most probable members, indicating a multiplicity fraction for this cluster of 25.6%+/-2%. We also observed field stars in the vicinity of the cluster and estimated a ratio of multiplicities of 286:17:1:0:0:0:1 (between one and seven companions), equivalent to a multiplicity fraction of 5.9%+/-3%. We showed that the cumulative distribution of separations for our sample stars is in agreement with Opik's law.</description><source format="bibcode">2015AJ....150...16G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/150/16</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+ 2001-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/280">I/280 : All-sky Compiled Catalogue of 2.5 million stars (Kharchenko+ 2009)</relatedResource><relatedResource 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