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<ri:Resource created="2014-06-24T10:55:02Z" 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>JHK and IRAC photometry of Sh2-90 YSOs</title><shortName>J/A+A/566/A122</shortName><identifier>ivo://CDS.VizieR/J/A+A/566/A122</identifier><altIdentifier>doi:10.26093/cds/vizier.35660122</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Samal M.R.</name></creator><creator><name>Zavagno A.</name></creator><creator><name>Deharveng L.</name></creator><creator><name>Molinari S.</name></creator><creator><name>Ojha D.K.</name></creator><creator><name>Paradis D.,Tige J.</name></creator><creator><name>Pandey A.K.</name></creator><creator><name>Russeil D.</name></creator><date role="Updated">2017-12-18T07:57:05Z</date><date role="Created">2014-06-24T10:55:02Z</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>h-ii-regions</subject><subject>young-stellar-objects</subject><subject>infrared-photometry</subject><description>We investigate the star formation activity in the molecular complex associated with the Galactic HII region Sh2-90. We obtain the distribution of the ionized and cold neutral gas using radio-continuum and Herschel observations. We use near-infrared and Spitzer data to investigate the stellar content of the complex. 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