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<ri:Resource created="2024-05-13T08:26:32Z" status="active" updated="2025-05-19T09:50:00Z" 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>Period variations of 32 contact binaries</title><shortName>J/AJ/167/18</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/18</identifier><altIdentifier>doi:10.26093/cds/vizier.51670018</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hong K.</name></creator><creator><name>Lee J.W.</name></creator><creator><name>Kim D.-J.</name></creator><creator><name>Park J.-H.</name></creator><creator><name>Kim H.-Y.</name></creator><creator><name>Rittipruk P.</name></creator><creator><name>Han C.</name></creator><date role="Updated">2024-11-06T20:19:44Z</date><date role="Created">2024-05-13T08:26:32Z</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>galactic-center</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We present detailed analyses of updated eclipse timing diagrams for 32 contact binary merger candidates in the Galactic bulge. The photometric data was obtained from 2016 to 2021 using the Korea Microlensing Telescope Network with the 1.6 m telescopes located at three southern sites (CTIO, SAAO, and SSO). The times of minimum lights were determined by applying the binary-star model to full light curves created at half-year intervals from the observations. The orbital period variations of the binary systems were analyzed using the O-C diagrams from our new timings with the others published in the literature, which are based on the OGLE observations from 2001 to 2015. As results, the orbital periods and period-decreasing rates of 32 binary systems were located to be in the ranges of 0.370 to 1.238 days and from -3.0 to -13.1x10^-6^day/yr, respectively. Out of these stars, 24 systems show a combination effect of a parabola and a light travel time caused by a third body, and their outer orbital periods are in the range of 9.1-26.5yr. We propose that all of our merger candidates need additional monitoring observations to study a luminous-red nova progenitor.</description><source format="bibcode">2024AJ....167...18H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/18</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/J/A+A/289/871">J/A+A/289/871 : YY Eri &amp; AE Phe (Maceroni+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/91">J/AJ/147/91 : Differential BVR light curves of V407 Peg (Lee+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/66/405">J/AcA/66/405 : Galactic bulge eclipsing &amp; ellipsoid binary (Soszynski+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/185">J/AJ/158/185 : 3 binary systems in the Large Magellanic Cloud (Hong+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/630/A75">J/A+A/630/A75 : Six luminous red novae photometry (Pastorello+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/157">J/AJ/163/157 : 14127 eclipsing binaries in the Galactic Bulge (Hong+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/164/202">J/AJ/164/202 : Extremely Low Mass Ratio Contact Binaries. 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