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<ri:Resource created="2026-07-15T14:49:16Z" status="active" updated="2026-07-15T14:28:42Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>BSN. II. Timing &amp; LCs of 8 eclipsing contact binaries</title><shortName>J/AJ/170/214</shortName><identifier>ivo://CDS.VizieR/J/AJ/170/214</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Poro A.</name></creator><creator><name>Li K.</name></creator><creator><name>Michel R.</name></creator><creator><name>Wang L.-H.</name></creator><creator><name>Alicavus F.</name></creator><creator><name>Najera M.R.,Santillan-Ortega P.</name></creator><creator><name>Tamayo F.J.</name></creator><creator><name>Aceves H.</name></creator><date role="Updated">2026-07-15T14:28:42Z</date><date role="Created">2026-07-15T14:49:16Z</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>multiple-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>This study provides the first comprehensive analysis of eight total-eclipse W Ursae Majoris-type contact binary systems. Ground-based photometric multiband observations were conducted at a Mexican observatory, and new times of minima were extracted. The O-C analysis reveals that four of our target binaries exhibit a long-term increase in their orbital periods, while the others show a long-term decrease in their orbital periods. We analyzed the light curves using the PHOEBE Python code and BSN application. Among the target systems, two required the inclusion of a cold starspot on one of the components to achieve an adequate fit. The light curve analysis revealed that the target systems exhibit a shallow fillout factor. Absolute parameters were estimated using the Gaia DR3 parallax and astrophysics equations. Considering the effective temperatures and component masses, each system was classified as either the A- or W-subtype. The stellar evolution of the systems was represented through the mass-radius and mass-luminosity diagrams. Additionally, we calculated the initial masses of the companion stars and the total mass lost for each target system.</description><source format="bibcode">2025AJ....170..214P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/170/214</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>IsServedBy</relationshipType><relatedResource>Conesearch 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-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/287">II/287 : Northern Sky Variability Survey (NSVS) (Wozniak+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</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/119/1901">J/AJ/119/1901 : ROTSE all-sky surveys for variable stars (Akerlof+, 2000)</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/ApJ/629/1055">J/ApJ/629/1055 : Evolution of close binary systems (Yakut+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/373/1483">J/MNRAS/373/1483 : W UMa type and CAB stars dynamical evolution (Eker+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/621">J/AJ/131/621 : A catalog of 1022 bright contact binary stars (Gettel+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/466">J/AJ/138/466 : NSVS variables automated classification (Hoffman+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/101">J/AJ/146/101 : LINEAR. 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