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ivo-id="ivo://CDS">CDS</publisher><creator><name>Wilson C.D.</name></creator><creator><name>Scoville N.</name></creator><creator><name>Madden S.C.</name></creator><creator><name>Charmandaris V.</name></creator><date role="Updated">2004-12-11T15:01:13Z</date><date role="Created">2004-12-11T16:00:28Z</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>molecular-clouds</subject><subject>co-line-emission</subject><subject>radio-galaxies</subject><description>We have used previously published observations of the CO emission from the Antennae (NGC 4038/4039) to study the detailed properties of the supergiant molecular complexes with the goal of understanding the formation of young massive star clusters.</description><source 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