A study of twelve potential merger candidate contact binary systems

Surjit S. Wadhwa, Bojan Arbutina, Nick F. H. Tothill, Miroslav D. Filipović, Ain Y. De Horta, Jelena Petrović, Gojko Djurašević

Research output: Contribution to journalArticlepeer-review

11 Citations (Scopus)

Abstract

Photometric 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.
Original languageEnglish
Article number74202
Number of pages9
JournalPublications of the Astronomical Society of the Pacific
Volume135
Issue number1049
Publication statusPublished - 1 Jul 2023

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© 2023. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP). All rights reserved.

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Original content from this work maybe used under the terms of the Creative Commons Attribution 3.0 licence (https://creativecommons.org/licenses/by/3.0/). Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

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