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<ri:Resource created="2018-04-06T14:21:48Z" status="active" updated="2025-06-13T15:25:00Z" 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>Orbit alignment in triple stars</title><shortName>J/ApJ/844/103</shortName><identifier>ivo://CDS.VizieR/J/ApJ/844/103</identifier><altIdentifier>doi:10.26093/cds/vizier.18440103</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tokovinin A.</name></creator><date role="Updated">2018-05-16T07:04:47Z</date><date role="Created">2018-04-06T14:21:48Z</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>orbits</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><description>The statistics of the angle {Phi} between orbital angular momenta in hierarchical triple systems with known inner visual or astrometric orbits are studied. A correlation between apparent revolution directions proves the partial orbit alignment known from earlier works. The alignment is strong in triples with outer projected separation less than ~50au, where the average {Phi} is about 20{deg}. In contrast, outer orbits wider than 1000 au are not aligned with the inner orbits. It is established that the orbit alignment decreases with the increasing mass of the primary component. The average eccentricity of inner orbits in well-aligned triples is smaller than in randomly aligned ones. These findings highlight the role of dissipative interactions with gas in defining the orbital architecture of low-mass triple systems. On the other hand, chaotic dynamics apparently played a role in shaping more massive hierarchies. The analysis of projected configurations and triples with known inner and outer orbits indicates that the distribution of {Phi} is likely bimodal, where 80% of triples have {Phi}&lt;70{deg} and the remaining ones are randomly aligned.</description><source format="bibcode">2017ApJ...844..103T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/844/103</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/J/AJ/111/370">J/AJ/111/370 : Orbits of 37 close visual systems (Hartkopf+ 1996)</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><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/341/121">J/A+A/341/121 : Visual binary orbits and masses (Soederhjelm 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/119/3084">J/AJ/119/3084 : ICCD speckle obs. of binary stars. 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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>WDS</name><description>WDS code (HHMMm+DDMM; J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType><flag>primary</flag></column><column><name>vo</name><description>Display the two known visual orbits (table 3)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Plx</name><description>[0.8/742.1] Hipparcos parallax</description><unit>mas</unit><ucd>pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M1</name><description>[0.05/50] Primary mass in the inner subsystem</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>P1</name><description>[0.1/3962.5] Inner period</description><unit>yr</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e1</name><description>Inner eccentricity</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a1</name><description>[0.001/32.4] Inner semimajor axis</description><unit>arcsec</unit><ucd>phys.angSize.smajAxis;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W1</name><description>[0/357] Inner node {Omega}_1_</description><unit>deg</unit><ucd>src.orbital.node</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>i1</name><description>[0/283] Inner inclination</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sep</name><description>[0.05/7860] Outer separation {rho}</description><unit>arcsec</unit><ucd>pos.angDistance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA</name><description>Outer position angle {theta}</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RevDir</name><description>[-1/1] Outer revolution direction (-1 for retrograde; 0 for unknown)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sign</name><description>[-1/1] Apparent revolution (1=corotating; -1=counter-rotating)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</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>Positions of component A in the WDS catalog (B/wds) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions of component A in the WDS catalog (B/wds) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/844/103/table3</name><description>Hierarchical systems with two known visual orbits</description><column><name>P</name><description>[0.01/1431] Period</description><unit>yr</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>I/O</name><description>Inner or outer subsystem</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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