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<ri:Resource created="2010-04-22T16:01:21Z" 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>NGC 2264 and ONC PMS stars in the infrared</title><shortName>J/ApJ/671/605</shortName><identifier>ivo://CDS.VizieR/J/ApJ/671/605</identifier><altIdentifier>doi:10.26093/cds/vizier.16710605</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cieza L.</name></creator><creator><name>Baliber N.</name></creator><date role="Updated">2018-01-04T08:22:41Z</date><date role="Created">2010-04-22T16:01:21Z</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>open-star-clusters</subject><subject>pre-main-sequence-stars</subject><subject>infrared-photometry</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>Observations of pre-main-sequence star rotation periods reveal slow rotators in young clusters of various ages, indicating that angular momentum is somehow removed from these rotating masses. The mechanism by which spin-up is regulated as young stars contract has been one of the longest standing problems in star formation. Attempts to observationally confirm the prevailing theory that magnetic interaction between the star and its circumstellar disk regulates these rotation periods have produced mixed results. In this paper, we use the unprecedented disk identification capability of the Spitzer Space Telescope to test the star-disk interaction paradigm in two young clusters, NGC 2264 and the Orion Nebula Cluster (ONC).</description><source format="bibcode">2007ApJ...671..605C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/671/605</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/2228">J/AJ/127/2228 : VRI photometry of PMS stars in NGC 2264 OB (Makidon+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/430/1005">J/A+A/430/1005 : VRIH{alpha} photometry of NGC 2264 variables (Lamm+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/113/1733">J/AJ/113/1733 : Orion Nebula Cluster population (Hillenbrand 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/1676">J/AJ/121/1676 : ONC low-mass stars photometry (Rebull+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/646/297">J/ApJ/646/297 : Spitzer observations of pre-main-sequence stars (Rebull+ 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/649/862">J/ApJ/649/862 : IR phot. of IC 348 pre-main-sequence stars (Cieza+, 2006)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/671/605</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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