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<ri:Resource created="2002-02-10T13:40:37Z" 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>NGC 2451A proper motions and membership</title><shortName>J/AJ/122/1486</shortName><identifier>ivo://CDS.VizieR/J/AJ/122/1486</identifier><altIdentifier>doi:10.26093/cds/vizier.51221486</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Platais I.</name></creator><creator><name>Kozhurina-Platais V.</name></creator><creator><name>Barnes S.</name></creator><creator><name>Girard T.M.</name></creator><creator><name>Demarque P.,van Altena W.F.</name></creator><creator><name>Deliyannis C.P.</name></creator><creator><name>Horch E.</name></creator><date role="Updated">2023-04-06T16:50:44Z</date><date role="Created">2002-02-10T13:40:37Z</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>open-star-clusters</subject><subject>proper-motions</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We provide new evidence that NGC 2451A is undoubtedly a young open cluster, although sparsely populated. New cluster membership has been derived from relative proper motions of 5868 stars. In total, 136 stars down to V~15 5 have membership probability P{mu}&gt;=2%. New CCD BV photometry indicates that about 70 stars are indeed main-sequence stars of NGC 2451A. This is also supported by our measurements of radial velocities. A total of 34 very likely cluster members yield a mean heliocentric radial velocity for NGC 2451A equal to +22.9km/s. The high quality of our BV photometry, a confirmation of cluster membership from proper motions and radial velocities, and a recently obtained metallicity estimate for several cluster stars allow us to perform a precise isochrone fit. The Yale isochrones, updated by the latest available input physics, have been fitted to the cluster's color-magnitude diagram, yielding a distance modulus V_0_-M_V_ in the range 6.35 to 6.38, which is in excellent agreement with the distance modulus (m-M)_0_=6.38 derived from the Hipparcos data recently by van Leeuwen and Robichon et al. (1998, Cat. &lt;J/A+AS/130/157&gt;). We have used the high-resolution spectra acquired using the Hydra multiobject spectrograph at the WIYN telescope (Kitt Peak, Arizona) in 1997 November and 1998 October.</description><source format="bibcode">2001AJ....122.1486P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/122/1486</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>http://www.astro.yale.edu/astrom : SPM Home Page</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/252">I/252 : The USNO-A2.0 Catalogue (Monet+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/277">I/277 : SPM catalog 2.0 (Platais+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/601">J/AJ/124/601 : WIYN Open Cluster Study. 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