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<ri:Resource created="2022-12-13T08:56:20Z" 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>UBVRI photometry of the eclipsing system V490 Sct</title><shortName>J/AJ/164/194</shortName><identifier>ivo://CDS.VizieR/J/AJ/164/194</identifier><altIdentifier>doi:10.26093/cds/vizier.51640194</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Volkov I.M.</name></creator><creator><name>Kravtsova A.S.</name></creator><date role="Updated">2023-01-16T09:14:14Z</date><date role="Created">2022-12-13T08:56:20Z</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>eclipsing-binary-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We report long-term UBVRIRcIc photometry of the highly eccentric 12.04 day detached eclipsing binary V490Sct (V=13.1, B9.5+A0,e=0.40), which we use to determine its relative and absolute parameters. The absolute masses, radii, and temperatures are MA=2.33{+/-}0.07M{sun}, RA=1.90{+/-}0.04R{sun}, and TA=9960{+/-}60K for the primary and MB=2.23{+/-}0.07M{sun}, RB=1.86{+/-}0.04R{sun}, and TB=9700{+/-}80K for the secondary. The system displays a slow periastron advance that is dominated by General Relativity (GR). Our measurement, {omega}=0.86deg/century, is 32% less then the expected rate, {omega}=1.24deg/century, which has an 83% contribution from GR. A comparison with current stellar evolution models shows a good match to the measured properties at an age of about 130Myr and Solar abundance. The photometric parallax of the system {pi}=0.73{+/-}0.04mas, matches the GAIA DR2 value, {pi}=0.76{+/-} 0.04mas.</description><source format="bibcode">2022AJ....164..194V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/164/194</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/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)</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/A+AS/141/371">J/A+AS/141/371 : Low-mass stars evolut. tracks &amp; isochrones (Girardi+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/424/919">J/A+A/424/919 : Stellar models grids. Z=0.02, M=0.8 to 125 (Claret, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/836/177">J/ApJ/836/177 : RVs and R-band obs. of the EB* V541 Cyg (Torres+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/41">J/ApJS/235/41 : Galactic EB stars eccentric orbits based on ETDs (Kim+, 2018)</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/164/194</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/164/194</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/164/194</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/164/194</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/164/194</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/164/194</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><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/164/194/table1</name><description>Observation log</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>ObsID</name><description>Observatory identifier</description><ucd>meta.id;instr.obsty</ucd><dataType xsi:type="vs:VOTableType" arraysize="57*">char</dataType></column><column><name>Tel</name><description>Telescope used</description><ucd>meta.id;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>Band</name><description>Photometric passband</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Equip</name><description>Receiving equipment</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column></table><table><name>J/AJ/164/194/table7</name><description>UBVRRcIIc photometry</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>Filt</name><description>Filter used (UBVRI)</description><ucd>instr.setup;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>HJD</name><description>[2453239/2459394] Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag</name><description>[12.1/14.7] Apparent magnitude in Filter</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>