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<ri:Resource created="2000-10-11T17:23:51Z" 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>Proper motion data of M10</title><shortName>J/A+AS/145/223</shortName><identifier>ivo://CDS.VizieR/J/A+AS/145/223</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen L.</name></creator><creator><name>Geffert M.</name></creator><creator><name>Wang J.J.</name></creator><creator><name>Reif K.</name></creator><creator><name>Braun J.M.</name></creator><date role="Updated">2000-10-11T17:24:38Z</date><date role="Created">2000-10-11T17:23:51Z</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>astrometry</subject><subject>globular-star-clusters</subject><subject>proper-motions</subject><description>We present the first proper motion study of M10 (NGC 6254). Absolute proper motions of about 532 stars in the field of the globular cluster M10 were determined with respect to Hipparcos and ACT reference stars. In addition to photographic plates of Bonn and Shanghai also wide field CCD observations as second epoch plates were used. The wide field CCD observations show an accuracy comparable to that of the photographic plates. A good coincidence of the solutions based on reference stars from Hipparcos and from ACT was found. Our final proper motions allow a sufficient separation of cluster and field stars. Two population II Cepheids were confirmed to be members of M10. The absolute proper motion of M10 was determined and combined with its distance from the Sun and its radial velocity. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CGW</name><description>Star sequence number (Cl* NGC 6254 CGW NNN in Simbad)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>RA2000</name><description>Right Ascension 2000 (hours)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE2000</name><description>Declination 2000 (degree)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>e_RAs</name><description>Error of Right Ascension</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_DEs</name><description>Error of Declination</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmRA</name><description>Proper motion in Right Ascension</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>Proper motion in Declination</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmRA</name><description>Error of proper motion in RA</description><unit>mas/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE</name><description>Error of proper motion in DE</description><unit>mas/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>