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<ri:Resource created="2012-07-27T14:59:17Z" 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>RV curves of Galactic massive O stars</title><shortName>J/other/Sci/337.</shortName><identifier>ivo://CDS.VizieR/J/other/Sci/337.444</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sana H.</name></creator><creator><name>de Mink S.E.</name></creator><creator><name>de Koter A.</name></creator><creator><name>Langer N.</name></creator><creator><name>Evans C.J.</name></creator><creator><name>Gieles M.,Gosset E.</name></creator><creator><name>Izzard R.G.</name></creator><creator><name>Le Bouquin J.-B.</name></creator><creator><name>Schneider F.R.N.</name></creator><date role="Updated">2017-10-11T05:13:40Z</date><date role="Created">2012-07-27T14:59:17Z</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>o-stars</subject><subject>radial-velocity</subject><description>The presence of a nearby companion alters the evolution of massive stars in binary systems, leading to phenomena such as stellar mergers, X-ray binaries and gamma-ray bursts. Unambiguous constraints on the fraction of massive stars affected by binary interaction were lacking. We simultaneously measured all relevant binary characteristics in a sample of Galactic massive O stars and quantified the frequency and nature of binary interactions. Over seventy per cent of all massive stars will exchange mass with a companion, leading to a binary merger in one third of the cases. 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