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<ri:Resource created="2014-11-14T15:23:04Z" 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>From binaries to multiples. II. Statistical data</title><shortName>J/AJ/147/87</shortName><identifier>ivo://CDS.VizieR/J/AJ/147/87</identifier><altIdentifier>doi:10.26093/cds/vizier.51470087</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tokovinin A.</name></creator><date role="Updated">2017-09-27T05:55:47Z</date><date role="Created">2014-11-14T15:23:04Z</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>dwarf-stars</subject><subject>f-stars</subject><subject>stellar-masses</subject><description>Statistics of hierarchical multiplicity among solar-type dwarfs are studied using the distance-limited sample of 4847 targets presented in the accompanying Paper I. Known facts about binaries (multiplicity fraction 0.46, lognormal period distribution with median period 100yr and logarithmic dispersion 2.4, and nearly uniform mass-ratio distribution independent of the period) are confirmed with a high statistical significance. The fraction of hierarchies with three or more components is 0.13+/-0.01, and the fractions of targets with n=1,2,3,... components are 54:33:8:4:1. Subsystems in the secondary components are almost as frequent as in the primary components, but in half of such cases both inner pairs are present. The high frequency of those 2+2 hierarchies (4%) suggests that both inner pairs were formed by a common process. The statistics of hierarchies can be reproduced by simulations, assuming that the field is a mixture coming from binary-rich and binary-poor environments. Periods of the outer and inner binaries are selected recursively from the same lognormal distribution, subject to the stability constraint and accounting for the correlation between inner subsystems. The simulator can be used to evaluate the frequency of multiple systems with specified parameters. However, it does not reproduce the observed excess of inner periods shorter than 10days, caused by tidal evolution.</description><source format="bibcode">2014AJ....147...87T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/147/87</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/141/52">J/AJ/141/52 : Low-mass visual companions to nearby G-dwarfs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/389/925">J/MNRAS/389/925 : Triple and quadruple stars (Tokovinin, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/450/681">J/A+A/450/681 : Companions to close spectroscopic binaries (Tokovinin+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/382/118">J/A+A/382/118 : Spectroscopic sub-systems in multiple stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/380/238">J/A+A/380/238 : Long-period companions of multiple stars (Shatsky, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/124/75">J/A+AS/124/75 : Multiple star catalogue (MSC) (Tokovinin 1997-1999)</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/AJ/147/87</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/147/87</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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67pc)</description><column><name>P1</name><description>Details of the system from Paper I (J/AJ/147/86, table 5)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">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>_RA</name><description>Position from Hipparcos (van Leeuwen 2007, I/311) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from Hipparcos (van Leeuwen 2007, I/311) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></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>HIP0</name><description>Hipparcos number of primary component</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>L</name><description>[1/121] Hierarchical level (1)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Type</name><description>Type of system (2)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>logP</name><description>? 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