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<ri:Resource created="2005-09-08T15:31:35Z" 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>The OB association LH 58</title><shortName>J/AJ/108/1256</shortName><identifier>ivo://CDS.VizieR/J/AJ/108/1256</identifier><altIdentifier>doi:10.26093/cds/vizier.51081256</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Garmany C.D.</name></creator><creator><name>Massey P.</name></creator><creator><name>Parker J.W.</name></creator><date role="Updated">2023-04-06T16:50:08Z</date><date role="Created">2005-09-08T15:31:35Z</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>stellar-associations</subject><subject>ccd-photometry</subject><description>We present CCD photometry and spectroscopy for stars in Lucke-Hodge 58, an isolated OB association in the Large Magellanic Cloud (LMC) northwest of 30 Doradus. The photometric catalog contains 839 stars with UBV magnitudes complete to V~19. We have obtained spectra and classified 35 stars; combined with previous published spectral types, we find 22 O-type stars. The earliest type is O3-4 V, and there are three WR stars in the association. The slope of the initial mass function, Gamma=-1.7+/-0.3, is in good agreement with other LMC associations. The presence of several evolved supergiants with masses about 15-25M_{sun}_ suggests that some star formation took place as early as 10 million years ago, but the majority of stars formed coevally within the past few million years. Addresses: Garmany C.D. garmany@jila.colorado.edu Joint Institute for Laboratory Astrophysics, Box 440 University of Colorado, Boulder, Colorado 80309-0389 Massey P. massey@noao.edu Kitt Peak National Observatory, National Optical Astronomy Observatories, P.O. 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