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<ri:Resource created="2014-12-02T07:45:15Z" 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>Photometry &amp; interferometry of nearby secondaries</title><shortName>J/AJ/148/72</shortName><identifier>ivo://CDS.VizieR/J/AJ/148/72</identifier><altIdentifier>doi:10.26093/cds/vizier.51480072</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tokovinin A.</name></creator><date role="Updated">2018-01-04T08:22:16Z</date><date role="Created">2014-12-02T07:45:15Z</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>photometry</subject><subject>interferometry</subject><description>To improve the statistics of hierarchical multiplicity, secondary components of wide nearby binaries with solar-type primaries were surveyed at the SOAR telescope for evaluating the frequency of subsystems. Images of 17 faint secondaries were obtained with the SOAR Adaptive Module that improved the seeing; one new 0.2'' binary was detected. For all targets, photometry in the g', i', z' bands is given. Another 46 secondaries were observed by speckle interferometry, resolving 7 close subsystems. Adding literature data, the binarity of 95 secondary components is evaluated. We found that the detection-corrected frequency of secondary subsystems with periods in the well-surveyed range from 10^3^ to 10^5^ days is 0.21+/-0.06--same as the normal frequency of such binaries among solar-type stars, 0.18. This indicates that wide binaries are unlikely to be produced by dynamical evolution of N-body systems, but are rather formed by fragmentation.</description><source format="bibcode">2014AJ....148...72T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/148/72</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/87">J/AJ/147/87 : From binaries to multiples. II. Statistical data</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/86">J/AJ/147/86 : From binaries to multiples. I. The FG-67 sample</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/422/14">J/MNRAS/422/14 : Radial velocities of wide doubles (Halbwachs+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/102">J/AJ/144/102 : Catalog of wide companions to HIP stars (Tokovinin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/525/A95">J/A+A/525/A95 : Search for brown-dwarf companions of stars (Sahlmann+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A52">J/A+A/509/A52 : Search for companions with VLT/NACO (Chauvin+, 2010)</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/450/681">J/A+A/450/681 : Companions to close spectroscopic binaries (Tokovinin+, 2006)</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/148/72</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/148/72</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/148/72</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/148/72</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/148/72</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/148/72</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/148/72/table3 (List of secondary components with high-resolution imaging data)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/148/72/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/148/72/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/148/72/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>31.8843</ra><dec>-59.6726</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/4128 4225 4241 4316 16930 18688 18711 20605 21076 21477 21519 21790 21829 21849 22043 22263 22479 22630 22679 23201 24628 24633 25099 25267 25397 25409 25660 25713 25728 26180 26217 26669 26680 26935 26956 27124 29653 33500 33552 33930 34199 34289 34626 36412 36889 36971 37074 37595 37714 37746 37763 37969 38076 38238 38433 38535 38936 39023 39031 39500 39557 39562 39730 39841 40293 40686 40901 41631 41701 41763 41861 42278 42465 42646 42656 42899 43072 43321 43680 43797 43998 44078 44123 44228 44920 45773 45865 47254 48022 48905</spatial><spectral>2.040811542443644e-19 4.653515163505597e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/148/72?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/148/72/table3</name><description>List of secondary components with high-resolution imaging data</description><column><name>Sub</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>SAM</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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