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<ri:Resource created="2019-10-22T09:05:26Z" 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>LL Com BVR bands photometry &amp; times of light minimum</title><shortName>J/AJ/158/104</shortName><identifier>ivo://CDS.VizieR/J/AJ/158/104</identifier><altIdentifier>doi:10.26093/cds/vizier.51580104</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hu K.</name></creator><creator><name>Chen K.</name></creator><creator><name>Xiang F.-Y.</name></creator><creator><name>Yu Y.-X.</name></creator><creator><name>Zhao E.-G.</name></creator><date role="Updated">2019-10-22T08:23:08Z</date><date role="Created">2019-10-22T09:05:26Z</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>Despite the discovery of LL Com, a Lyrae-type eclipsing binary system, approximately 60 yr ago, little has been found concerning its detailed photometry and orbital-period change until now. In this paper, we present the first multi-band charge-coupled-device photometric light curves, from which a significant luminosity reduction around the primary eclipse is revealed. Based on LAMOST data, we first determined LL Com's spectrum as F1V and then analyzed the light curves with the 2015 version of the Wilson-Devinney code. The fact that LL Com is a near-contact binary system with a semi-detached configuration, where the secondary component only fills its Roche lobe and the primary component fills more than 95% of its Roche lobe, is suggested through the photometric solution. In addition, according to archival photometry and previously published times of minima, a secular period increase at a rate of P=2.62x10^-7^ day/yr was found, which implies a continuous mass transfer from the secondary to the primary. Utilizing the photometric solution and the simulations of single-particle trajectories, we propose the existence of a cool spot on the surface of the primary component. This cool spot can be naturally produced by the impacts that occur during mass flow, and it also successfully interprets the luminosity reduction in the light curves. Finally, with the combination of thermal relaxation oscillation theory and the Roche-Lobe model, we conclude that LL Com is transitioning from the semi-detached to the detached phase.</description><source format="bibcode">2019AJ....158..104H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/158/104</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/other/IBVS/5296">J/other/IBVS/5296 : Extrema of pulsating stars (Agerer+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5438">J/other/IBVS/5438 : 162-nd list of minima of eclipsing binaries</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/54/207">J/AcA/54/207 : Ephemerids of eclipsing binaries (Kreiner, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5543">J/other/IBVS/5543 : 163-nd list of minima of eclipsing binaries</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5802">J/other/IBVS/5802 : Minima and maxima of 735 variables (Hubscher+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1067">J/AJ/136/1067 : New beta Lyrae and Algol candidates in NSVS</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5918">J/other/IBVS/5918 : Minima and maxima of 452 variables (Hubscher+, 2010)</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/158/104</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/158/104</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/158/104</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/158/104</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/158/104</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/158/104</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>Infrared</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/158/104/table2</name><description>BVR bands photometric data for the eclipsing binary LL Com</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>HJD-B</name><description>Heliocentric Julian Date of B band observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase-B</name><description>[0.001/0.999] Corresponding phase for HJD of B band</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DBmag</name><description>[-0.672/-0.078] Differential B band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_DBmag</name><description>[0.002/0.01] Photometric error in DBmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HJD-V</name><description>Heliocentric Julian Date of V band observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase-V</name><description>[0/0.998] Corresponding phase for HJD of V band</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DVmag</name><description>[-0.604/-0.049] Differential V band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_DVmag</name><description>[0.002/0.007] Photometric error in DVmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HJD-R</name><description>? Heliocentric Julian Date of R band observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Phase-R</name><description>[0.001/0.999]? Corresponding phase for HJD of R band</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DRmag</name><description>[-0.574/-0.043]? Differential R band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_DRmag</name><description>[0.002/0.006]? Photometric error in DRmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/AJ/158/104/table4</name><description>Times of light minimum of LL Com</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>HJD-Min</name><description>Heliocentric Julian Date of light-minimum time</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_HJD-Min</name><description>[0.0001/0.0047]? Corresponding error for HJD-Min</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Type</name><description>Type of light minimum (I=Primary; II=Secondary)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Meth</name><description>[pg ccd] Method of observation (1)</description><ucd>meta.code;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Ref</name><description>[1/44] Reference (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>