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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1313
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dc.contributor.authorWadhwa, Surjit S.en_US
dc.contributor.authorArbutina, Bojanen_US
dc.contributor.authorTothill, Nick F.H.en_US
dc.contributor.authorFilipović, Miroslav D.en_US
dc.contributor.authorDe Horta, Ain Y.en_US
dc.contributor.authorPetrović, Jelenaen_US
dc.contributor.authorDjurašević, Gojkoen_US
dc.date.accessioned2024-07-05T06:23:24Z-
dc.date.available2024-07-05T06:23:24Z-
dc.date.issued2023-07-01-
dc.identifier.issn00046280-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/1313-
dc.description.abstractPhotometric observations and analysis of twelve previously poorly studied contact binary systems is presented. All show total eclipses and have extremely low mass ratios ranging from 0.072 to 0.15. Also, all show characteristics of orbital instability with mass ratios within the theoretical orbital instability range. Although none demonstrate a significant O’Connell effect at least nine of the systems have other indicators of increased chromospheric and magnetic activity.en_US
dc.language.isoenen_US
dc.publisherIOP Scienceen_US
dc.relation.ispartofPublications of the Astronomical Society of the Pacificen_US
dc.rightsAttribution 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/us/*
dc.subjectContact binary starsen_US
dc.subjectOrbital elementsen_US
dc.subjectTransient detectionen_US
dc.titleA Study of Twelve Potential Merger Candidate Contact Binary Systemsen_US
dc.typeArticleen_US
dc.identifier.doi10.1088/1538-3873/ace3f5-
dc.identifier.scopus2-s2.0-85166108447-
dc.identifier.isi001030299400001-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85166108447-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0004-6280en_US
dc.description.rankM21en_US
dc.relation.firstpageArticle no. 074202en_US
dc.relation.volume135en_US
dc.relation.issue1049en_US
item.fulltextWith Fulltext-
item.languageiso639-1en-
item.openairetypeArticle-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-8036-4132-
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