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<ri:Resource created="2023-07-31T08:30:51Z" 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>Evidence for disc regulation in NGC 2264</title><shortName>J/MNRAS/487/2937</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/487/2937</identifier><altIdentifier>doi:10.26093/cds/vizier.74872937</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Orcajo S.</name></creator><creator><name>Cieza L.A.</name></creator><creator><name>Gamen R.</name></creator><creator><name>Peterson D.</name></creator><date role="Updated">2025-05-06T20:13:58Z</date><date role="Created">2023-07-31T08:30:51Z</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>late-type-stars</subject><subject>variable-stars</subject><subject>stellar-spectral-types</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><description>In the pre-main-sequence stage, star-disc interactions have been shown to remove stellar angular momentum and regulate the rotation periods of stars with M2 and earlier spectral types. Whether disc regulation also extends to stars with later spectral types still remains a matter of debate. Here, we present a star-disc interaction study in a sample of over 180 stars with spectral types M3 and later (corresponding to stellar masses &lt;=0.3M_{sun}_) in young stellar cluster NGC 2264. Combining rotation periods from the literature, new and literature spectral types, and newly presented deep Spitzer observations, we show that stars with masses below 0.3M_{sun}_ with discs also rotate slower than stars without a disc in the same mass regime. Our results demonstrate that disc regulation still operates in these low-mass stars, although the efficiency of this process might be lower than in higher mass objects. We confirm that stars with spectral types earlier and later than M2 have distinct period distributions and that stars with spectral types M5 and later rotate even faster M3 and M4-type stars.</description><source format="bibcode">2019MNRAS.487.2937O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/487/2937</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/114/2644">J/AJ/114/2644 : UBVRIHa photometry of NGC2264 (Sung+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1117">J/AJ/127/1117 : Halpha emission-line stars in NGC2264 (Reipurth+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/590/A78">J/A+A/590/A78 : NGC2264 weak-line T Tauri lithium abundances (Bouvier+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/609/A10">J/A+A/609/A10 : NGC2264 structure and star formation history (Venuti+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/8">J/ApJ/821/8 : Spectroscopic binary population of ONC and NGC2264</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/670/A37">J/A+A/670/A37 : Spatial and dynamical structure of NGC2264 (Flaccomio+, 2023)</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/MNRAS/487/2937</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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