Published January 1, 2018
| Version v1
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Searching for planets around eclipsing binary stars using timing method: NSVS 14256825
Creators
- 1. Ataturk Univ, Dept Astron & Astrophys, Erzurum, Turkey
- 2. N Copernicus Univ, Fac Phys Astron & Appl Informat, Torun, Poland
- 3. Univ Zielona Gora, Janusz Gil Inst Astron, Zielona Gora, Poland
- 4. Jagiellonian Univ, Astron Observ, Krakow, Poland
Description
We present four new mid eclipse times and an updated O-C diagram of the short period eclipsing binary NSVS14256825. The new data follow the (O-C) trend and its model proposed in Nasiroglu et al. (2017). The (O-C) diagram shows quasi-periodic variations that can be explained with the presence of a brown-dwarf in a quasi-circular circumbinary orbit.
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