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<ri:Resource created="2018-03-06T11:28:38Z" 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>Praesepe members rotational periods from K2 LCs</title><shortName>J/ApJ/842/83</shortName><identifier>ivo://CDS.VizieR/J/ApJ/842/83</identifier><altIdentifier>doi:10.26093/cds/vizier.18420083</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Douglas S.T.</name></creator><creator><name>Agueros M.A.</name></creator><creator><name>Covey K.R.</name></creator><creator><name>Kraus A.</name></creator><date role="Updated">2018-05-14T09:13:25Z</date><date role="Created">2018-03-06T11:28:38Z</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>late-type-stars</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>multiple-stars</subject><subject>infrared-photometry</subject><description>We analyze K2 light curves for 794 low-mass (1&gt;~M_*_&gt;~0.1M_{sun}_) members of the ~650Myr old open cluster Praesepe and measure rotation periods (P_rot_) for 677 of these stars. We find that half of the rapidly rotating &gt;~0.3M_{sun}_ stars are confirmed or candidate binary systems. The remaining &gt;~0.3M_{sun}_ fast rotators have not been searched for companions, and are therefore not confirmed single stars. We previously found that nearly all rapidly rotating 0.3M_{sun}_ stars in the Hyades are binaries, but we require deeper binary searches in Praesepe to confirm whether binaries in these two co-eval clusters have different P_rot_ distributions. We also compare the observed P_rot_ distribution in Praesepe to that predicted by models of angular-momentum evolution. We do not observe the clear bimodal P_rot_ distribution predicted by Brown (2014ApJ...789..101B) for &gt;0.5M_{sun}_ stars at the age of Praesepe, but 0.25-0.5M_{sun}_ stars do show stronger bimodality. In addition, we find that &gt;60% of early M dwarfs in Praesepe rotate more slowly than predicted at 650Myr by Matt+ (2015ApJ...799L..23M), which suggests an increase in braking efficiency for these stars relative to solar-type stars and fully convective stars. The incompleteness of surveys for binaries in open clusters likely impacts our comparison with these models since the models only attempt to describe the evolution of isolated single stars.</description><source format="bibcode">2017ApJ...842...83D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/842/83</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/sb9">B/sb9 : SB9: 9th Catalogue of Spectroscopic Binary Orbits (Pourbaix+ 2004-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/521/682">J/ApJ/521/682 : Binaries in the Praesepe and Coma clusters (Abt+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/375/989">J/A+A/375/989 : JHK photometry of Praesepe low-mass stars (Bouvier+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/1570">J/AJ/123/1570 : alpha Persei and Praesepe Clusters (Patience+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/1570">J/AJ/124/1570 : JHKs photometry in Praesepe (Adams+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/2340">J/AJ/134/2340 : Praesepe &amp; Coma Berenices cluster membership (Kraus+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/907">J/AJ/135/907 : Variables in Praesepe identified with KELT (Pepper+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/498/949">J/A+A/498/949 : Velocities of F-K dwarfs in open clusters (Mermilliod+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/166">J/AJ/141/166 : HATNet variability survey of K and M dwarfs (Hartman+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/413/2218">J/MNRAS/413/2218 : Stellar rotation in Hyades and Praesepe (Delorme+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/L33">J/ApJ/756/L33 : RVs of 2 hot Jupiters in Praesepe (Quinn+, 2012)</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/MNRAS/442/2081">J/MNRAS/442/2081 : Praesepe members light curves (Kovacs+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/795/161">J/ApJ/795/161 : Activity &amp; rotation in Praesepe &amp; the Hyades (Douglas+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/588/A118">J/A+A/588/A118 : Pr0211 RVs, photom. and activity indexes (Malavolta+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/822/47">J/ApJ/822/47 : K2 rotation periods for 65 Hyades members (Douglas+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/594/A100">J/A+A/594/A100 : K2 new planetary and EB candidates (Barros+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/113">J/AJ/152/113 : Pleiades members with K2 LCs. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Literature name if any (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>EPIC</name><description>EPIC identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>Mass</name><description>[0.1/1.5] Mass from Paper II, Table 5 (2014, J/ApJ/795/161)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r'mag</name><description>[9.1/23.6] r' mag from Paper II, Table 5 (2014, J/ApJ/795/161)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>[8.4/15.4] K band mag from Paper II, Table 5 (2014, J/ApJ/795/161)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Prot1</name><description>[0.1/38.1]? Rotational Period, first periodogram peak</description><unit>d</unit><ucd>time.period;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pw1</name><description>[0.007/1]? Power, first periodogram peak</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Q1</name><description>[0/3]? Q flag, first periodogram peak (0=confirmed detection) (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Clean?</name><description>[YN ] There are no peaks &gt;60% of the primary peak's power</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Sig</name><description>[0.005/0.02]? Minimum significance thresholds for the periodogram peaks</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Prot2</name><description>[0.1/27.1]? Rotational Period, second periodogram peak</description><unit>d</unit><ucd>time.period;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pw2</name><description>[0.009/0.4]? Power, second periodogram peak</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Q2</name><description>[0/1]? Q flag, second periodogram peak (0=confirmed detection) (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MP?</name><description>[YMN ] Multiple rotational periods? (M:maybe)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SE?</name><description>[YMN ] Spot evolution? Y:yes, M:maybe, N:no</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Bl?</name><description>[YMN ] Blend? Y:yes, M:maybe, N:no</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Bin?</name><description>Binary status: conf=confirmed; cand=candidate</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>RawAmp</name><description>[0.0009/0.3]? Photometric amplitude of variability (2)</description><unit>mag</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SmAmp</name><description>[0.005/11]? Smoothed amplitude of variability (3)</description><unit>%</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>P</name><description>Period selected as the final period to plot (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>ProtA</name><description>[0.5/36]? PTF Rotational Period from Agueros+ (2011ApJ...740..110A)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProtD</name><description>[2.4/14.6]? SWASP Rotational Period from Delorme+ (2011, J/MNRAS/413/2218)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProtS</name><description>[0.2/6]? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Literature name if any (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>EPIC</name><description>? EPIC identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column><column><name>ProtA</name><description>[1.5/25.4]? PTF, rotational period, from Agueros+ (2011ApJ...740..110A) (1)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProtD</name><description>[2.4/10]? SWASP rotational period from Delorme+ (2011, J/MNRAS/413/2218) (1)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProtS</name><description>[0.2/6]? Rotational period from Scholz+ (2007MNRAS.381.1638S, 2011MNRAS.413.2595S) (1)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ProtK</name><description>[5.8/19.2]? Rotational period from Kovacs+ (2014, J/MNRAS/442/2081) (1)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Prot</name><description>[0.4/18.3]? K2 rotational period; this work</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PrCat</name><description>Display data from Kovacs+, 2014, J/MNRAS/442/2081 and Delorme+, 2011, J/MNRAS/413/2218, within 3"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>PCat</name><description>Data from Kraus and Hillenbrand (2007, J/AJ/134/2340) and Adams+ (2002, J/AJ/124/1570) within 3"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>All</name><description>Display all data for this source in this catalog (tables 1-3)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</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><table><name>J/ApJ/842/83/table2</name><description>Companions to Praesepe members with measured Prot</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Triple</name><description>Triple Type</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Refs</name><description>Source References (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="93*">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>Name</name><description>Literature name if any (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>EPIC</name><description>? EPIC identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column><column><name>2MASS</name><description>2MASS Identifer (JHHMMSSss+DDMMSSs) if any</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>RAJ2000</name><description>[8] Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[16/25] Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Epoch</name><description>[2000] Epoch of position</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Binary</name><description>Binary Type</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>PCat</name><description>Data from Kraus and Hillenbrand (2007, J/AJ/134/2340) and Adams+ (2002, J/AJ/124/1570) within 3"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>All</name><description>Display all data for this source in this catalog (tables 1-3)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>