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Catalog of W UMa type binary systems with additional components based on eclipsing time variations
Institution:1. Department of Space Sciences and Technologies, Faculty of Arts and Sciences, Çanakkale Onsekiz Mart University, Terzio?lu Kampüsü, Çanakkale TR-17020, Turkey;2. Department of Physics, Faculty of Arts and Sciences, Çanakkale Onsekiz Mart University, Terzio?lu Kampüsü, Çanakkale TR-17020, Turkey;3. Çanakkale Onsekiz Mart University, Astrophysics Research Centre and Ulup?nar Observatory, Çanakkale TR-17020, Turkey;1. Department of Applied Mathematics, University of Western Ontario, London, ON, N6A 5B7, Canada;2. Department of Physics & Astronomy, University of Western Ontario, London, ON, N6A 3K7, Canada;1. Department of Physical Science and Technology, Kunming University, Kunming 650214, China;2. Department of Astronomy, Yunnan University, Kunming 650091, China;1. The International Occultation Timing Association Middle East section, Iran;2. Adana Organised Industrial Zones Vocational School of Technical Science, University of Çukurova, 01410, Adana, Turkey;3. Space Science and Solar Energy Research and Application Center (UZAYMER), University of Çukurova, 01330, Adana, Turkey;1. School of Physics and Mechanical & Electrical Engineering, Hubei University of Education, Wuhan 430205, China;2. Research Center for Astronomy, Hubei University of Education, Wuhan 430205, China;3. Institute of Astrophysics, Central China Normal University, Wuhan 430079, China
Abstract:A catalog of W UMa type eclipsing binary systems with tertiary components based on eclipse timing diagrams is presented listing the physical and orbital parameters (including third body parameters) of 150 W UMa type eclipsing binaries.In this study, the (O–C) diagrams of nine sample W UMa type eclipsing binary systems, based on the most reliable timings of minima in the literature, are analyzed to obtain the third-body parameters and significant statistical results are presented from the data in the catalog.
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