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<ri:Resource created="1997-12-09T18:01:39Z" status="active" updated="2025-06-13T15:25:00Z" 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>UBV photometry of V360 Lac</title><shortName>J/A+A/324/965</shortName><identifier>ivo://CDS.VizieR/J/A+A/324/965</identifier><altIdentifier>doi:10.26093/cds/vizier.33240965</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hill G.</name></creator><creator><name>Harmanec P.</name></creator><creator><name>Pavlovski K.</name></creator><creator><name>Bozic H.</name></creator><creator><name>Hadrava P.</name></creator><creator><name>Koubsky P.,Ziznovsky J.</name></creator><date role="Updated">1997-12-09T17:01:42Z</date><date role="Created">1997-12-09T18:01:39Z</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>be-stars</subject><subject>spectroscopic-binary-stars</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><description>An analysis of an extensive collection of photometric and spectroscopic observations of the little studied bright Be star V360 Lac lead to the following main conclusions: (1) V360 Lac is a binary system consisting of a B3e primary and a F9IV secondary which probably fills the Roche lobe and losses mass towards the primary. Radial-velocity curves of both components were obtained. (2) The light variations arise from superposition of variations on at least three time scales: phase-locked orbital brightness and colour changes with two minima; sinusoidal variation with a 322.24^d^ period and low-amplitude rapid changes with a possible period of 1.6738^d^. (3) A tentative solution of the B and V light curves which assumes the semi-detached configuration and presence of a disk around the primary, combined with the orbital solution, leads to preliminary basic physical elements of the system which are consistent with the radiative properties of the binary components.</description><source format="bibcode">1997A&amp;A...324..965H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/324/965</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/J/A+A/328/551">J/A+A/328/551 : Spectroscopic data of 4 Herculis. Paper 18. (Koubsky+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/387/580">J/A+A/387/580 : UBV photometry of V832 Cyg. Paper 21. (Harmanec+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/416/669">J/A+A/416/669 : UBV photometry of HD 6226. Paper 22. (Bozic+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/419/607">J/A+A/419/607 : Long-term variations of kappa Dra. Paper 23. (Saad+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/459/849">J/A+A/459/849 : Radial velocities of ups Sgr. Paper 25 (Koubsky+, 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/A+A/324/965</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/324/965</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/324/965</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/324/965</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/324/965</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/324/965</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/A+A/324/965/table4</name><description>V360 Lac: individual homogenized Johnson UBV observations from several stations</description><column><name>w</name><description>weight of the data point</description><ucd>stat.weight</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>? Johnson V magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag</name><description>Johnson B magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Umag</name><description>? Johnson U magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.U</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>HJD</name><description>Heliocentric Julian date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B-V</name><description>? Johnson B-V index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>U-B</name><description>? Johnson U-B index</description><unit>mag</unit><ucd>phot.color;em.opt.U;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>X</name><description>Air mass of the observation</description><ucd>obs.airMass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dX</name><description>Air mass difference between var. and comp.</description><ucd>obs.airMass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HD</name><description>HD number of the comparison star used</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Obs</name><description>Numerical code identifying sources of data (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>