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<ri:Resource created="2010-03-10T17:38:19Z" 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>S3MC: YSOs in N66, in SMC</title><shortName>J/ApJ/669/327</shortName><identifier>ivo://CDS.VizieR/J/ApJ/669/327</identifier><altIdentifier>doi:10.26093/cds/vizier.16690327</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Simon J.D.</name></creator><creator><name>Bolatto A.D.</name></creator><creator><name>Whitney B.A.</name></creator><creator><name>Robitaille T.P.</name></creator><creator><name>Shah R.Y.,Makovoz D.</name></creator><creator><name>Stanimirovic S.</name></creator><creator><name>Barba R.H.</name></creator><creator><name>Rubio M.</name></creator><date role="Updated">2010-03-10T16:47:27Z</date><date role="Created">2010-03-10T17:38:19Z</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>young-stellar-objects</subject><description>We use Spitzer Space Telescope observations from the Spitzer Survey of the Small Magellanic Cloud (S^3^MC) to study the young stellar content of N66, the largest and brightest HII region in the SMC. In addition to large numbers of normal stars, we detect a significant population of bright, red infrared sources that we identify as likely to be young stellar objects (YSOs). 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