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<ri:Resource created="2012-09-27T09:22:28Z" 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>Spectral classification of stars in NGC 6530</title><shortName>J/A+A/546/A9</shortName><identifier>ivo://CDS.VizieR/J/A+A/546/A9</identifier><altIdentifier>doi:10.26093/cds/vizier.35460009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Prisinzano L.</name></creator><creator><name>G. Micela</name></creator><creator><name>S. Sciortino</name></creator><creator><name>L. Affer</name></creator><creator><name>F. Damiani</name></creator><date role="Updated">2017-06-20T13:16:46Z</date><date role="Created">2012-09-27T09:22:28Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>morgan-keenan-classification</subject><subject>effective-temperature</subject><description>Mechanisms involved in the star formation process and in particular the duration of the different phases of the cloud contraction are not yet fully understood. Photometric data alone suggest that objects coexist in the young cluster NGC 6530 with ages from ~1Myr up to 10Myrs. 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