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<ri:Resource created="2010-12-22T09:45:20Z" 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>CHARA observations of 3 late-type stars</title><shortName>J/ApJ/683/424</shortName><identifier>ivo://CDS.VizieR/J/ApJ/683/424</identifier><altIdentifier>doi:10.26093/cds/vizier.16830424</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boyajian T.S.</name></creator><creator><name>McAlister H.A.</name></creator><creator><name>Baines E.K.</name></creator><creator><name>Gies D.R.</name></creator><creator><name>Henry T.</name></creator><creator><name>Jao W.-C.,O'Brien D.</name></creator><creator><name>Raghavan D.</name></creator><creator><name>Touhami Y.</name></creator><creator><name>ten Brummelaar T.A.</name></creator><creator><name>Farrington C.,Goldfinger P.J.</name></creator><creator><name>Sturmann L.</name></creator><creator><name>Sturmann J.</name></creator><creator><name>Turner N.H.</name></creator><creator><name>Ridgway S.</name></creator><date role="Updated">2014-10-20T15:14:43Z</date><date role="Created">2010-12-22T09:45:20Z</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>late-type-stars</subject><subject>interferometry</subject><description>Using the longest baselines of the CHARA Array, we have measured the angular diameter of the G5V subdwarf {mu} Cas A, the first such determination for a halo population star. We compare this result to new diameters for the higher metallicity K0V stars, {sigma} Dra and HR 511, and find that the metal-poor star, {mu} Cas A, has an effective temperature (T_eff_=5297+/-32K), radius (R=0.791+/-0.008R_{sun}_), and absolute luminosity (L=0.442+/-0.014L_{sun}_) comparable to those of the other two stars with later spectral types. We show that stellar models show a discrepancy in the predicted temperature and radius for {mu} Cas A, and we discuss these results and how they provide a key to understanding the fundamental relationships for stars with low metallicity.</description><source format="bibcode">2008ApJ...683..424B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/683/424</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/VI/46">VI/46 : Second Catalog of Interferometric Measurements of Binary Stars</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/ApJ/683/424</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/683/424</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/683/424</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/683/424</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/683/424</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/683/424</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>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/683/424/table1</name><description>Interferometric measurements</description><column><name>V</name><description>Visibility (1)</description><ucd>phot.flux;arith.ratio</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>HR</name><description>HR (Bright Star) number of star</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd></column><column><name>JD</name><description>Julian Date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B</name><description>Projected baseline</description><unit>m</unit><ucd>instr.baseline</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>psi</name><description>Orientation of the baseline on the sky</description><unit>deg</unit><ucd>obs.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_V</name><description>The 1{sigma} error in V</description><ucd>stat.error;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>