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<ri:Resource created="2022-02-21T06:20:10Z" 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>Stellar spins in the open cluster NGC 2516</title><shortName>J/ApJ/903/99</shortName><identifier>ivo://CDS.VizieR/J/ApJ/903/99</identifier><altIdentifier>doi:10.26093/cds/vizier.19030099</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Healy B.F.</name></creator><creator><name>McCullough P.R.</name></creator><date role="Updated">2022-09-30T23:05:24Z</date><date role="Created">2022-02-21T06:20:10Z</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>visible-astronomy</subject><subject>radial-velocity</subject><subject>stellar-radii</subject><subject>effective-temperature</subject><description>Measuring the distribution of stellar spin axis orientations in a coeval group of stars probes the physical processes underlying the stars' formation. In this paper, we use spectrophotometric observations of the open cluster NGC2516 to determine the degree of spin alignment among its stars. We combine TESS light curves, ground-based spectroscopy from the Gaia-ESO and GALAH surveys, broadband stellar magnitudes from several surveys, and Gaia astrometry to measure 33 stellar inclinations and quantify overall cluster rotation. Our measurements suggest that stellar spins in this cluster are isotropically oriented, while allowing for the possibility that they are moderately aligned. An isotropic distribution of NGC2516 spins would imply a star-forming environment in which turbulence dominated ordered motion, while a moderately aligned distribution would suggest a more substantial contribution from rotation. We also perform a three-dimensional analysis of the cluster's internal kinematics, finding no significant signatures of overall rotation. Stemming from this analysis, we identify evidence of cluster contraction, suggesting possible ongoing mass segregation in NGC2516.</description><source format="bibcode">2020ApJ...903...99H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/903/99</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/B/simbad">B/simbad : Simbad objects catalogue (M.Wenger 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/360/472">J/A+A/360/472 : Proper motions in omega Centauri (van Leeuwen+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/375/863">J/A+A/375/863 : Photometry in NGC 2516 (Jeffries+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/290">J/AJ/123/290 : UBVI CCD photometry of NGC 2516 (Sung+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/398/647">J/A+A/398/647 : Rotational velocities of F and G stars (Reiners+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/402/1380">J/MNRAS/402/1380 : Rotation velocities Pleiades &amp; {alpha}Per (Jackson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/432/1203">J/MNRAS/432/1203 : Rotation periods of M-dwarf stars (McQuillan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/L10">J/A+A/557/L10 : Rotation periods of 12000 Kepler stars (Nielsen+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/776/67">J/ApJ/776/67 : Rotational tracks (van Saders+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/150/97">J/AJ/150/97 : Radial velocities M67. 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