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<ri:Resource created="2015-07-01T09:17:32Z" 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>Robo-AO observations of binary stars</title><shortName>J/ApJ/799/4</shortName><identifier>ivo://CDS.VizieR/J/ApJ/799/4</identifier><altIdentifier>doi:10.26093/cds/vizier.17990004</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Riddle R.L.</name></creator><creator><name>Tokovinin A.</name></creator><creator><name>Mason B.D.</name></creator><creator><name>Hartkopf W.I.</name></creator><creator><name>Roberts L.C.JR,Baranec C.</name></creator><creator><name>Law N.M.</name></creator><creator><name>Bui K.</name></creator><creator><name>Burse M.P.</name></creator><creator><name>Das H.K.</name></creator><creator><name>Dekany R.G.,Kulkarni S.</name></creator><creator><name>Punnadi S.</name></creator><creator><name>Ramaprakash A.N.</name></creator><creator><name>Tendulkar S.P.</name></creator><date role="Updated">2018-05-30T07:07:27Z</date><date role="Created">2015-07-01T09:17:32Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>multiple-stars</subject><description>We conducted a survey of nearby binary systems composed of main sequence stars of spectral types F and G in order to improve our understanding of the hierarchical nature of multiple star systems. Using Robo-AO, the first robotic adaptive optics instrument, we collected high angular resolution images with deep and well-defined detection limits in the Sloan Digital Sky Survey i' band. A total of 695 components belonging to 595 systems were observed. We prioritized observations of faint secondary components with separations over 10" to quantify the still poorly constrained frequency of their subsystems. Of the 214 secondaries observed, 39 contain such subsystems; 19 of those were discovered with Robo-AO. The selection-corrected frequency of secondary subsystems with periods from 10^3.5^ to 10^5^ days is 0.12+/-0.03, the same as the frequency of such companions to the primary. Half of the secondary pairs belong to quadruple systems where the primary is also a close pair, showing that the presence of subsystems in both components of the outer binary is correlated. The relatively large abundance of 2+2 quadruple systems is a new finding, and will require more exploration of the formation mechanism of multiple star systems. We also targeted close binaries with periods less than 100 yr, searching for their distant tertiary components, and discovered 17 certain and 2 potential new triples. In a subsample of 241 close binaries, 71 have additional outer companions. The overall frequency of tertiary components is not enhanced, compared to all (non-binary) targets, but in the range of outer periods from 10^6^ to 10^7.5^ days (separations on the order of 500AU), the frequency of tertiary components is 0.16+/-0.03, exceeding the frequency of similar systems among all targets (0.09) by almost a factor of two. Measurements of binary stars with Robo-AO allowed us to compute first orbits for 9 pairs and to improve orbits of another 11 pairs.</description><source format="bibcode">2015ApJ...799....4R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/799/4</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/B/sb9">B/sb9 : SB9: 9th Catalogue of Spectroscopic Binary Orbits (Pourbaix+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/322">I/322 : UCAC4 Catalogue (Zacharias+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/123">J/AJ/147/123 : Speckle interferometry with SOAR in 2012-2013 (Tokovinin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/86">J/AJ/147/86 : From binaries to multiples I. 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The (O-C) residual in PA</description><unit>deg</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>(O-C)r</name><description>? The (O-C) residual in rho</description><unit>arcsec</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ref</name><description>? Reference code (see refs.dat file)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></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 Simbad with HIP number) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position (from Simbad with HIP number) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/799/4/table5</name><description>New pairs resolved with Robo-AO</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>WDS</name><description>WDS designation (HHMMm+DDMM; J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>No</name><description>Number of observations for this system</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>HIP</name><description>Hipparcos number of the primary component in each system</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Disc</name><description>Discoverer designation</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>N</name><description>[1/5] Number of observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</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>rho</name><description>[0.09/39] Separation</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dmag</name><description>[0/7] Magnitude difference between components</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>u_Dmag</name><description>Uncertainty flag on Dmag</description><ucd>meta.code.error;arith.diff</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Notes</name><description>Status and remarks (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="50*">char</dataType></column></table><table><name>J/ApJ/799/4/refs</name><description>References</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>Ref</name><description>Reference code</description><ucd>meta.note;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>BibCode</name><description>Bibcode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Aut</name><description>Author's name(s)</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>Comm</name><description>Comment</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="46*">char</dataType></column></table></schema></tableset></ri:Resource>