CAOSP abstracts, Volume: 50, No.: 4, year: 2020

Author(s): Zervas, K.; Christopoulou, E.-P.; Papageorgiou, A.
Journal: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 50, no. 4, p. 772-773.
Date: 11/2020
Title: Substellar and stellar companions in eclipsing binaries
Keyword(s): binaries: eclipsing, binaries (including multiple): close, planetary systems
Pages: 772 -- 773
DOI: https://doi.org/10.31577/caosp.2020.50.4.772
NASA ADS Abstract Service: 2020CoSka..50..772Z
Citation:
License: This work is licensed under a Creative Commons Attribution 4.0 International License

Abstract: We present an extensive analysis of O-C diagrams constructed by previously published times of minima and updated by photometric observations carried out at Mythodea Observatory (Astrophysics Laboratory, Department of Physics, University of Patras). A two-companion model is attributed to the over-contact (W UMa type) binary system TZ Boo according to a Light-Time Effect (LITE), while in the case of the post-common envelope binary NSVS 14256825 a Jovian type circumbinary companion is the most plausible explanation of the apparent period variation.

Note:
This paper was presented at the conference "Universe of Binaries, Binaries in the Universe" held in Telč, Czech Republic, September 7-11, 2019.