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<ri:Resource created="1999-10-18T13:18:58Z" 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>Open star clusters. I. NGC 581 (M 103)</title><shortName>J/A+A/349/448</shortName><identifier>ivo://CDS.VizieR/J/A+A/349/448</identifier><altIdentifier>doi:10.26093/cds/vizier.33490448</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sanner J.</name></creator><creator><name>Geffert M.</name></creator><creator><name>Brunzendorf J.</name></creator><creator><name>Schmoll J.</name></creator><date role="Updated">1999-10-18T13:19:33Z</date><date role="Created">1999-10-18T13:18:58Z</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>ccd-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>proper-motions</subject><description>We present CCD photometry and a proper motion study of the young open star cluster, NGC 581 (M 103). Fitting isochrones to the colour magnitude diagram, we found an age of 16+/-4Myr and a distance of roughly 3kpc for this cluster. The proper motion study identifies 77 stars of V=14.5mag or brighter to be cluster members. We combine membership determination by proper motions and statistical field star subtraction to derive the IMF of the cluster and find a quite steep slope of {Gamma}=-1.80.</description><source format="bibcode">1999A&amp;A...349..448S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/349/448</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/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/357/471">J/A+A/357/471 : Open star clusters. II. 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