A Study of Twelve Potential Merger Candidate Contact Binary Systems

被引：11
作者：
Wadhwa, Surjit S. [1 ]
Arbutina, Bojan [2 ]
Tothill, Nick F. H. [1 ]
Filipovic, Miroslav D. [1 ]
De Horta, Ain Y. [1 ]
Petrovic, Jelena [3 ]
Djurasevic, Gojko [3 ]
机构：
[1] Western Sydney Univ, Sch Sci, Locked Bag 1797, Penrith, NSW 2751, Australia
[2] Univ Belgrade, Fac Math, Dept Astron, Studentski Trg 16, Belgrade 11000, Serbia
[3] Astron Observ, Volgina 7, Belgrade 11060, Serbia
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 2023年 / 135卷 / 1049期
关键词：
MASS-RATIO; VARIABLE-STARS; COBITOM PROJECT; ORBITAL PERIOD; LIGHT CURVES; EVOLUTION; PROGENITOR; SUNSPOTS; CATALOG; LIBRARY;
D O I：
10.1088/1538-3873/ace3f5
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
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收藏
页数：9
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