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<ri:Resource created="2004-07-24T14:12:32Z" 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>JHKs photometry in N159 (LMC)</title><shortName>J/A+A/422/129</shortName><identifier>ivo://CDS.VizieR/J/A+A/422/129</identifier><altIdentifier>doi:10.26093/cds/vizier.34220129</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Meynadier F.</name></creator><creator><name>Heydari-Malayeri M.</name></creator><creator><name>Deharveng L.</name></creator><creator><name>Charmandaris V.,Le Bertre T.</name></creator><creator><name>Rosa M.R.</name></creator><creator><name>Schaerer D.</name></creator><creator><name>Zinnecker H.</name></creator><date role="Updated">2004-07-24T14:13:11Z</date><date role="Created">2004-07-24T14:12:32Z</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>magellanic-clouds</subject><subject>h-ii-regions</subject><subject>early-type-stars</subject><subject>infrared-photometry</subject><description>We study the Large Magellanic Cloud Papillon Nebula (N 159-5), a conspicuous High Excitation Blob (HEB) lying in the star forming complex N 159. Using JHK near-infrared photometry obtained at the ESO VLT with the ISAAC camera, we examine the stellar populations associated with the Papillon, tracing their history using stellar evolution models. Two populations are revealed: one composed of young, massive stars with an age ~3Myr, and a second consisting of older lower mass stars of age spreading between 1 and 10Gyr. We analyze the properties of those populations and discuss their significance in the context of N 159. 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