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<ri:Resource created="2025-02-25T16:04:10Z" status="active" updated="2026-02-10T20:05:37Z" 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>Rot. vel. &amp; inclinations in stars of open clusters</title><shortName>J/ApJ/944/39</shortName><identifier>ivo://CDS.VizieR/J/ApJ/944/39</identifier><altIdentifier>doi:10.26093/cds/vizier.19440039</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Healy B.F.</name></creator><creator><name>McCullough P.R.</name></creator><creator><name>Schlaufman K.C.</name></creator><creator><name>Kovacs G.</name></creator><date role="Updated">2026-02-10T20:05:37Z</date><date role="Created">2025-02-25T16:04:10Z</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>stellar-radii</subject><subject>two-color-diagrams</subject><subject>effective-temperature</subject><subject>visible-astronomy</subject><description>We analyze spectroscopic and photometric data to determine the projected inclinations of stars in 11 open clusters, placing constraints on the spin-axis distributions of six clusters. We combine these results with four additional clusters studied by Healy &amp; McCullough (Paper I; 2020, J/ApJ/903/99) and Healy+ (Paper II; 2021, J/ApJ/923/23) to perform an ensemble analysis of their spins. We find that eight out of 10 constrained clusters (80%) have spin-axis orientations consistent with isotropy, and we establish a lower limit of four out of 10 (40%) isotropic clusters at 75% confidence, assuming no correlation of spins between clusters. We also identify two clusters whose spin-axis distributions can be better described by a model consisting of an aligned fraction of stars combined with an isotropic distribution. However, the inclination values of these stars may be influenced by systematic error, and the small number of stars modeled as aligned in these two clusters precludes the interpretation that their stellar subsets are physically aligned. Overall, no cluster displays an unambiguous signature of spin alignment, and 97% of the stars in our sample are consistent with isotropic orientations in their respective clusters. Our results offer support for the dominance of turbulence over ordered rotation in clumps and do not suggest the alignment of rotation axes and magnetic fields in protostars.</description><source format="bibcode">2023ApJ...944...39H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/944/39</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/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : 2MASS All-Sky Extended Source Catalog (XSC) (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/335">II/335 : Revised cat. of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/365">II/365 : CatWISE2020 catalog (updated version 28-Jan-2021) (Marocco+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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Source of vsini measurements (2)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Thresh</name><description>[5/12]? vsini threshold we established for each data set (see Section 3.4)</description><unit>km/s</unit><ucd>phys.veloc.rotat;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType><flag>nullable</flag></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</flag></column><column><name>Ns</name><description>Number of stars for this cluster (link to Table 3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Ninc</name><description>Number of inclinations measurements for stars in this cluster (link to Table 4)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>CG18</name><description>Display data from Cantat-Gaudin+ 2018, J/A+A/618/A93 within 14'</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>PapII</name><description>Display data from Paper II (Healy+ 2021, J/ApJ/923/23)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/944/39/table3</name><description>TESS-based rotation periods of stars in targeted clusters</description><column><name>GaiaDR2</name><description>Gaia DR2 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>PMm</name><description>[0.1/1] Membership probability</description><ucd>stat.probability;meta.code.member</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bp-Rp</name><description>[-0.18/3.7] Gaia DR2 Blue minus Red passband color</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>[0.22/14.6] Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Per</name><description>[0.0028/3.8] Uncertainty in Per</description><unit>d</unit><ucd>stat.error;time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Cluster</name><description>Cluster identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GaiaEDR3</name><description>Gaia EDR3 source identifier</description><ucd>meta.id.cross</ucd></column><column><name>TIC</name><description>[4154225/818505977] TESS Input Catalog identifier</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>RA_ICRS</name><description>Gaia EDR3 Right Ascension (ICRS) at Epoch=2016</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>[-61.7/59.1] Gaia EDR3 Declination (ICRS) at Epoch=2016</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/944/39/table4</name><description>Relevant quantities and determinations of the inclinations of open cluster members</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GaiaDR2</name><description>Gaia DR2 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>GaiaEDR3</name><description>Gaia EDR3 source identifier</description><ucd>meta.id.cross</ucd></column><column><name>TIC</name><description>[4205889/464839176] TESS Input Catalog identifier</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>Teff</name><description>[3182/15000] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[5/700] Uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>[0.37/2.72] Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rad</name><description>[0.0015/0.05] Uncertainty in Rad</description><unit>solRad</unit><ucd>stat.error;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vsini</name><description>[5/124.2] Projected rotational velocity</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Cluster</name><description>Cluster identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>e_vsini</name><description>[0.2/17] Uncertainty in vsini</description><unit>km/s</unit><ucd>stat.error;phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>[0.2/10] Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Per</name><description>[0.0003/1.7] Uncertainty in Per</description><unit>d</unit><ucd>stat.error;time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>sini</name><description>[0.048/2] Sine of the inclination</description><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_sini</name><description>[0.01/1] Upper uncertainty in sini</description><ucd>stat.error;stat.max;src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_sini</name><description>[0.0079/1] Lower uncertainty in sini</description><ucd>stat.error;stat.min;src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>