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<ri:Resource created="2013-01-09T16:16:37Z" 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>NAO Rozhen CCD measurements of multiple stars</title><shortName>J/AJ/142/73</shortName><identifier>ivo://CDS.VizieR/J/AJ/142/73</identifier><altIdentifier>doi:10.26093/cds/vizier.51420073</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cvetkovic Z.</name></creator><creator><name>Pavlovic R.</name></creator><creator><name>Damljanovic G.</name></creator><creator><name>Boeva S.</name></creator><date role="Updated">2018-01-04T08:22:29Z</date><date role="Created">2013-01-09T16:16:37Z</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><description>Using the 2m telescope of the Bulgarian National Astronomical Observatory at Rozhen, observations of 145 double or multiple stars were carried out during three nights on 2010 September 7-9. This is the fifth series of measurements of CCD frames of double and multiple stars obtained at Rozhen. In this paper, we present the results for the position angle and angular separation for 202 pairs and residuals for 45 pairs with published orbital elements or linear solutions. These observations have angular separations in the range 1.150"-196.372", with a median angular separation of 57.906". 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