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<ri:Resource created="2015-11-13T08:07:45Z" status="active" updated="2025-06-13T15:25:00Z" 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>KMOS view of the Galactic centre. I.</title><shortName>J/A+A/584/A2</shortName><identifier>ivo://CDS.VizieR/J/A+A/584/A2</identifier><altIdentifier>doi:10.26093/cds/vizier.35840002</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Feldmeier-Krause A.</name></creator><creator><name>Neumayer N.</name></creator><creator><name>Schoedel R.</name></creator><creator><name>Seth A.</name></creator><creator><name>Hilker M.,de Zeeuw P.T.</name></creator><creator><name>Kuntschner H.</name></creator><creator><name>Walcher C.J.</name></creator><creator><name>Luetzgendorf N.,Kissler-Patig M.</name></creator><date role="Updated">2017-07-05T14:24:04Z</date><date role="Created">2015-11-13T08:07:45Z</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>early-type-stars</subject><subject>emission-line-stars</subject><subject>wolf-rayet-stars</subject><subject>radial-velocity</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>The Galactic centre hosts a crowded, dense nuclear star cluster with a half-light radius of 4pc. Most of the stars in the Galactic centre are cool late-type stars, but there are also &gt;=100 hot early-type stars in the central parsec of the Milky Way. These stars are only 3-8Myr old. Our knowledge of the number and distribution of early-type stars in the Galactic centre is incomplete. Only a few spectroscopic observations have been made beyond a projected distance of 0.5pc of the Galactic centre. 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