In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 50, no. 4
K. Zervas - E.-P. Christopoulou - A. Papageorgiou
Details:
Year, pages: 2020, 772 - 773
Language: eng
Keywords:
binaries: eclipsing, binaries (including multiple): close, planetary systems
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2020/Vol_50/No_4/pp772-773_abstract.html
About article:
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.
How to cite:
ISO 690:
Zervas, K., Christopoulou, E., Papageorgiou, A. 2020. Substellar and stellar companions in eclipsing binaries. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 50, no.4, pp. 772-773. 1335-1842. DOI: https://doi.org/10.31577/caosp.2020.50.4.772
APA:
Zervas, K., Christopoulou, E., Papageorgiou, A. (2020). Substellar and stellar companions in eclipsing binaries. Contributions of the Astronomical Observatory Skalnaté Pleso, 50(4), 772-773. 1335-1842. DOI: https://doi.org/10.31577/caosp.2020.50.4.772
About edition:
Publisher: Astronomical Institute, Slovak Academy of Sciences
Published: 1. 11. 2020
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