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<ri:Resource created="2017-06-26T06:42:29Z" 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>Eccentricity distribution of wide binaries</title><shortName>J/MNRAS/456/2070</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/456/2070</identifier><altIdentifier>doi:10.26093/cds/vizier.74562070</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tokovinin A.</name></creator><creator><name>Kiyaeva O.</name></creator><date role="Updated">2024-08-15T20:17:21Z</date><date role="Created">2017-06-26T06:42:29Z</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><description>A sample of 477 solar-type binaries within 67pc with projected separations larger than 50AU is studied by a new statistical method. Speed and direction of the relative motion are determined from the short observed arcs or known orbits, and their joint distribution is compared to the numerical simulations. By inverting the observed distribution with the help of simulations, we find that average eccentricity of wide binaries is 0.59+/-0.02 and the eccentricity distribution can be modelled as f(e)~1.2e+0.4. However, wide binaries containing inner subsystems, i.e. triple or higher order multiples, have significantly smaller eccentricities with the average e=0.52+/-0.05 and the peak at e~0.5. We find that the catalogue of visual orbits is strongly biased against large eccentricities. A marginal evidence of eccentricity increasing with separation (or period) is found for this sample. Comparison with spectroscopic binaries proves the reality of the controversial period-eccentricity relation. The average eccentricity does increase with binary period, being 0.39 for periods from 10^2^ to 10^3^d and 0.59 for the binaries studied here (10^5^-10^6^d).</description><source format="bibcode">2016MNRAS.456.2070T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/456/2070</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/wds">B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 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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>HIP</name><description>Hipparcos number of primary component</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Type</name><description>[LCO] Type of motion from Table 2</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>t0</name><description>Reference epoch (1)</description><unit>yr</unit><ucd>meta.ref;time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>theta0</name><description>Position angle at moment t0</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_theta0</name><description>? rms uncertainty on theta0 (1)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>theta1</name><description>Speed of angular motion</description><unit>deg/yr</unit><ucd>pos.pm;phys.veloc.ang</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_theta1</name><description>? rms uncertainty on theta1 (1)</description><unit>deg/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>rho0</name><description>Separation at moment t0</description><unit>arcsec</unit><ucd>pos.angDistance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_rho0</name><description>? rms uncertainty on rho0 (1)</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>rho1</name><description>Speed of radial motion</description><unit>arcsec/yr</unit><ucd>pos.angDistance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_rho1</name><description>? rms uncertainty on rho1 (1)</description><unit>arcsec/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mu</name><description>Speed of relative motion</description><unit>mas/yr</unit><ucd>phys.veloc;src.orbital.meanMotion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_mu</name><description>? rms uncertainty on mu (1)</description><unit>mas/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>gamma</name><description>Angle of relative motion w.r.t. radius</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_gamma</name><description>? rms uncertainty on gamma (1)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mu1</name><description>Normalized relative motion (1)</description><ucd>phys.veloc;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DeltaT</name><description>? 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