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<ri:Resource created="2018-05-29T07:07:04Z" 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>The multiplicity of M dwarfs in young moving groups</title><shortName>J/ApJ/846/93</shortName><identifier>ivo://CDS.VizieR/J/ApJ/846/93</identifier><altIdentifier>doi:10.26093/cds/vizier.18460093</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shan Y.</name></creator><creator><name>Yee J.C.</name></creator><creator><name>Bowler B.P.</name></creator><creator><name>Cieza L.A.</name></creator><creator><name>Montet B.T.</name></creator><creator><name>Canovas H.,Liu M.C.</name></creator><creator><name>Close L.M.</name></creator><creator><name>Hinz P.M.</name></creator><creator><name>Males J.R.</name></creator><creator><name>Morzinski K.M.</name></creator><creator><name>Vaz A.,Bailey V.P.</name></creator><creator><name>Follette K.B. (The MagAO Team)</name></creator><date role="Updated">2018-07-19T12:25:07Z</date><date role="Created">2018-05-29T07:07:04Z</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>multiple-stars</subject><subject>infrared-photometry</subject><subject>stellar-spectral-types</subject><subject>proper-motions</subject><subject>stellar-masses</subject><subject>stellar-distance</subject><description>We image 104 newly identified low-mass (mostly M-dwarf) pre-main sequence (PMS) members of nearby young moving groups (YMGs) with Magellan Adaptive Optics (MagAO) and identify 27 stellar binaries with instantaneous projected separation as small as 40mas. Fifteen were previously unknown. The total number of multiple systems in this sample including spectroscopic and visual binaries from the literature is 36, giving a raw stellar multiplicity rate of at least 35_-4_^+5^% for this population. In the separation range of roughly 1-300au in which infrared AO imaging is most sensitive, the raw multiplicity rate is at least 24_-4_^+5^% for binaries resolved by the MagAO infrared camera (Clio). The M-star subsample of 87 stars yields a raw multiplicity of at least 30_-4_^+5^% over all separations, 21_-4_^+5^% for secondary companions resolved by Clio from 1 to 300au (23_-4_^+5^% for all known binaries in this separation range). A combined analysis with binaries discovered by the Search for Associations Containing Young stars shows that stellar multiplicity fraction as a function of mass over the range of 0.2 to 1.2M_{sun}_ appears to be linearly flat, in contrast to the field, where multiplicity increases with mass. After bias corrections are applied, the multiplicity of low-mass YMG members (0.2-0.6M_{sun}_) is in excess of the field. The overall multiplicity fraction is also consistent with being constant in age and across YMGs, which suggests that multiplicity rates for this mass range are largely set by 10Myr without appreciable evolution thereafter.</description><source format="bibcode">2017ApJ...846...93S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/846/93</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/322">I/322 : UCAC4 Catalogue (Zacharias+, 2012)</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/356/541">J/A+A/356/541 : T Tauri stars in the Sco-Cen OB association (Koehler+, 2000)</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/other/ARA+A/42.685">J/other/ARA+A/42.685 : Young stars near the Sun (Zuckerman+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/173/104">J/ApJS/173/104 : Stellar population in Chamaeleon I (Luhman, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/696/L84">J/ApJ/696/L84 : Primordial circumstellar disks in binaries (Cieza+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A52">J/A+A/509/A52 : Search for companions with VLT/NACO (Chauvin+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/1">J/ApJS/190/1 : A survey of stellar families (Raghavan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/44">J/ApJ/754/44 : The AstraLux Large M-dwarf Survey (Janson+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/745/19">J/ApJ/745/19 : Binary systems in Taurus-Auriga (Kraus+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/762/88">J/ApJ/762/88 : Young stellar kinematic group cand. members (Malo+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/435/1325">J/MNRAS/435/1325 : Membership of the {epsilon} Cha association (Murphy+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A26">J/A+A/568/A26 : SACY. 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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>YMG</name><description>Abbreviated YMG name</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>AName</name><description>Abbreviated target name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>SpT</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Dist</name><description>[16/120] Distance</description><unit>pc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Dist</name><description>[1/19] Error in distance</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Epoch</name><description>Best epoch of observation</description><ucd>time.epoch;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Band</name><description>Band (H or Ks (1 occurrence))</description><ucd>meta.code;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Sep</name><description>[0.05/3.2] Angular separation</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Sep</name><description>[0/0.03] Error on Sep</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA</name><description>[8/326] Position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PA</name><description>[0.3/4.5] Error on PA</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dMag</name><description>[0.03/5.1] Delta-magnitude</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dMag</name><description>[0.01/0.3] Error on dMag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CoMv</name><description>Comoving flag (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Punbd</name><description>[0/0.08] Unbound probability</description><unit>%</unit><ucd>stat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PSep</name><description>[1.1/281.4] Projected physical separation</description><unit>AU</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PSep</name><description>[0.1/16.1] Error on PSep</description><unit>AU</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mp</name><description>[0.1/0.9]? 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