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<ri:Resource created="2023-03-30T09:15:08Z" 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>EBs in Ruprecht 147. IV. EPIC 219511354 LCs &amp; RVs</title><shortName>J/ApJ/921/133</shortName><identifier>ivo://CDS.VizieR/J/ApJ/921/133</identifier><altIdentifier>doi:10.26093/cds/vizier.19210133</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Torres G.</name></creator><creator><name>Vanderburg A.</name></creator><creator><name>Curtis J.L.</name></creator><creator><name>Kraus A.L.</name></creator><creator><name>Gaidos E.</name></creator><date role="Updated">2023-10-16T11:55:14Z</date><date role="Created">2023-03-30T09:15:08Z</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>eclipsing-binary-stars</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><description>We report follow-up spectroscopic observations of the 1.62 day, K-type, detached, active, near-circular, double-lined eclipsing binary EPIC 219511354 in the open cluster Ruprecht 147, identified previously on the basis of photometric observations from the Kepler/K2 mission. This is the fourth eclipsing system analyzed in this cluster. A combined analysis of the light curve and radial velocities yields accurate masses of M_Aa_=0.912+/-0.013M_{sun}_ and M_Ab_=0.822+/-0.010M_{sun}_ for the primary (star Aa) and secondary (Ab), along with radii of R_Aa_=0.920+/-0.016R_{sun}_ and R_Ab_=0.851+/-0.016R_{sun}_, and effective temperatures of 5035+/-150 and 4690+/-130K, respectively. Comparison with current models of stellar evolution for the known age and metallicity of the cluster reveals that both radii are larger (by 10%-14%) and both temperatures cooler (by ~6%) than theoretically predicted, as is often seen in M dwarfs. This is likely caused by the significant stellar activity in the system, manifested here by 6% peak- to-peak out-of-eclipse variability, a filled-in H{alpha} line, and its detection as an X-ray source. We also find EPIC 219511354 to be a hierarchical triple system, with a low-mass tertiary in an eccentric 220 day orbit.</description><source format="bibcode">2021ApJ...921..133T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/921/133</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/469/355">J/ApJ/469/355 : Teff, B-V and BC relation (Flower, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/1144">J/AJ/124/1144 : Orbits of single-lined spectroscopic binaries (Latham, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/450/681">J/A+A/450/681 : Companions to close sp. binaries (Tokovinin+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/662/602">J/ApJ/662/602 : Radial velocities of HD 110555 (Torres+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A54">J/A+A/512/A54 : Teff and Fbol from Infrared Flux Method (Casagrande+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/A+ARV/18.67">J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/A75">J/A+A/529/A75 : Limb-darkening coefficients (Claret+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/742/123">J/ApJ/742/123 : Photometry and Velocity of LSPM J1112+7626 (Irwin+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/134">J/AJ/145/134 : RVels of 108 stars in Ruprecht 147 (Curtis+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/454/2863">J/MNRAS/454/2863 : Teff against colours calibrations (Huang+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/8">J/AJ/152/8 : Stellar multiplicity on planetary systems I. 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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>BJD</name><description>[57301.48/57382.81] Barycentric Julian Date; BJD-2400000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RFluxNF</name><description>[0.59/1.01] Not Flattened residual flux (1)</description><ucd>stat.fit.residual;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJ/921/133/table2</name><description>Heliocentric Radial Velocity Measurements of EPIC 219511354</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>BJD</name><description>[57297.69/59384.9] Barycentric Julian Date; BJD-2400000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVAa</name><description>[-62.1/151.5] Radial velocity of component Aa</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVAa</name><description>[1.26/2.15] RVAa uncertainty</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RVAb</name><description>[-72.2/157.4] Radial velocity of component Ab</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVAb</name><description>[2.03/3.5] RVAb uncertainty</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Inner</name><description>[0.11/0.95] Inner phase</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Outer</name><description>[0.12/1] Outer phase</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>