Abstract
The O – C diagram for the eclipsing binary system TY Boo was constructed with the new minima times observed at the Ankara University Observatory along with the collected ones from the literature. The O – C diagram shows a cyclic variation superimposed on a quadratic variation. The quadratic variation can be explained in terms of mass loss/exchange mechanism in the system while the cyclic variation is attributed to a possible light-time effect caused by a third body revolving around the close binary.
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Elmash, A., Selam, S.O., Albayrak, B., Özuyar, D. (2006). Possible Light-Time Effect in the Eclipsing Binary System TY Boo. In: Giménez, À., Guinan, E., Niarchos, P., Rucinski, S. (eds) Close Binaries in the 21st Century: New Opportunities and Challenges. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5027-5_46
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DOI: https://doi.org/10.1007/978-1-4020-5027-5_46
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Online ISBN: 978-1-4020-5027-5
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