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<ri:Resource created="2017-02-03T09:42:00Z" 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>BV(RI)c light curves of FF Vul</title><shortName>J/AJ/152/199</shortName><identifier>ivo://CDS.VizieR/J/AJ/152/199</identifier><altIdentifier>doi:10.26093/cds/vizier.51520199</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Samec R.G.</name></creator><creator><name>Nyaude R.</name></creator><creator><name>Caton D.</name></creator><creator><name>Van Hamme W.</name></creator><date role="Updated">2017-06-26T11:49:32Z</date><date role="Created">2017-02-03T09:42:00Z</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>High-precision BVR_c_I_c_ light curves of FF Vul were taken during the fall of 2015 with the Dark Sky Observatory 0.81m reflector of Appalachian State University, and the SARA north 0.91m reflector at KPNO. FF Vul is an eclipsing binary with a period of 0.44 day. A Wilson-Devinney solution shows that the binary is a near-contact, semidetached binary, i.e., with a V1010 Oph-type configuration. Five eclipse timings (three primary and two secondary) were calculated. A quadratic ephemeris was determined indicating that the period is decreasing. A near-equatorial hot spot was modeled on the cooler, secondary star, possibly caused by matter impacting from the primary component via the inner Lagrangian point. The component temperature difference is more than 1500K. The solution confirms a total secondary eclipse of 23 minutes duration. As expected in binaries of this type, there is a magnetic spot region.</description><source format="bibcode">2016AJ....152..199S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/152/199</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/vsx">B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/334/860">J/AN/334/860 : Catalogue of eclipsing variables. Version 2 (Avvakumova+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1067">J/AJ/136/1067 : New beta Lyrae and Algol candidates in NSVS (Hoffman+, 2008)</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/152/199</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/152/199</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/152/199</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/152/199</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/152/199</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/152/199</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/152/199/table1</name><description>Observations of FF Vul</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>Flt</name><description>[BVRI] Filter (Johnson-Cousins B, V, R_c_, or I_c_)</description><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>HJD</name><description>[7.5/40.8] Modified Heliocentric Julian Date (HJD-2457270)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dmag</name><description>[-0.22/0.84] The {Delta} magnitude in Flt (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>