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<ri:Resource created="2015-06-12T15:00:49Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Spectroscopy of the quadruple system HD 91962</title><shortName>J/AJ/149/195</shortName><identifier>ivo://CDS.VizieR/J/AJ/149/195</identifier><altIdentifier>doi:10.26093/cds/vizier.51490195</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tokovinin A.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Mason B.D.</name></creator><date role="Updated">2017-06-21T08:22:40Z</date><date role="Created">2015-06-12T15:00:49Z</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>x-ray-sources</subject><subject>radial-velocity</subject><description>The young nearby solar-type star HD 91962 is a rare quadruple system where three companions revolve around the main component with periods of 170.3days, 8.85years, and 205years. The two outer orbits are nearly co-planar, and all orbits have small eccentricities. We refine the visual orbit of the outer pair and determine the combined spectro-interferometric orbit of the middle 8.8year pair and the spectroscopic orbit of the inner binary. The middle and inner orbits are likely locked in a 1:19 resonance, and the ratio of the outer and middle periods is ~23. The masses of all components are estimated (inside-out: 1.14, 0.32, 0.64, 0.64 solar mass). The dynamical parallax is 27.4+/-0.6mas. We speculate that this multiple system originated from collapse of an isolated core and that the companions migrated in a dissipative disk. Other multiple systems with similar features (co-planarity, small eccentricity, and period ratio around 20) are known.</description><source format="bibcode">2015AJ....149..195T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/149/195</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/123">J/AJ/147/123 : 2012/2013 speckle interferometry with SOAR (Tokovinin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/87">J/AJ/147/87 : From binaries to multiples. II. (Tokovinin, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/743">J/AJ/139/743 : Speckle interferometry in 2008-09 (Tokovinin+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/181/62">J/ApJS/181/62 : Survey of young solar analogs (Metchev+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/1099">J/A+A/493/1099 : CaII HK emission in rapidly rotating stars (Schroeder+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2524">J/AJ/133/2524 : Spectra of young nearby stars (White+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/356/141">J/A+A/356/141 : BV photometry for components of HIP doubles (Fabricius+ 2000)</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/149/195</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/149/195</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/149/195</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/149/195</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/149/195</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/149/195</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>X-ray</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/149/195/speckle</name><description>Speckle measurements and residuals for the systems Aa,Ab , and A,B</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>Comp</name><description>Component (Aa,Ab or A,B</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Year</name><description>[1903/2016] Besselian year</description><unit>yr</unit><ucd>time</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PA</name><description>[0/360] Position angle {theta}</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sep</name><description>[0/2] Separation {rho}</description><unit>arcsec</unit><ucd>pos.angDistance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Sep</name><description>Assumed error used for weighting</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(O-C)PA</name><description>The (O-C) residual in position angle</description><unit>deg</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(O-C)Sep</name><description>The (O-C) residual in separation</description><unit>arcsec</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/149/195/table4</name><description>Radial velocities and residuals of Aa1,Aa2 (P=170.304+/-0.013d)</description><column><name>O-C</name><description>The (O-C) residual</description><unit>km/s</unit><ucd>stat.fit.residual;stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType">float</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>JD</name><description>[48290/56828] Julian Date (JD-2400000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RV</name><description>[8.3/35] Radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RV</name><description>[0.1/0.6] Uncertainty in RV</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>