Searching for planets around eclipsing binary stars using timing method: NSVS 14256825

Nasıroğlu, İlham; GOZDZIEWSKI, Krzysztof; Slowikowska, Aga; KRZESZOWSKİ, Krzysztof; ZEJMO, Michal; Zola, Staszek; Er, Hüseyin

doi:10.1017/s1743921317005658

Bildiri Tam Metin Bildiri Uluslararası 2017

Searching for planets around eclipsing binary stars using timing method: NSVS 14256825

İlham Nasıroğlu, Krzysztof GOZDZIEWSKI, Aga Slowikowska, Krzysztof KRZESZOWSKİ, Michal ZEJMO, Staszek Zola, Hüseyin Er

330th Symposium of the International-Astronomical-Union (IAU) ss. 405–406 · Nice · 24.04.2017–28.04.2017 · 24.04.2017

DOI ile aç

Özet

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.

Atıf için künye

Nasıroğlu, İ., GOZDZIEWSKI, K., Slowikowska, A., KRZESZOWSKİ, K., ZEJMO, M., Zola, S., & Er, H. (2017). Searching for planets around eclipsing binary stars using timing method: NSVS 14256825. 330th Symposium of the International-Astronomical-Union (IAU), Nice (ss. 405–406). https://doi.org/10.1017/s1743921317005658

BibTeX

@inproceedings{nasiroglu2017-62225,
  author = {Nasıroğlu, İlham and GOZDZIEWSKI, Krzysztof and Slowikowska, Aga and KRZESZOWSKİ, Krzysztof and ZEJMO, Michal and Zola, Staszek and Er, Hüseyin},
  title = {Searching for planets around eclipsing binary stars using timing method: NSVS 14256825},
  booktitle = {330th Symposium of the International-Astronomical-Union (IAU)},
  address = {Nice},
  year = {2017},
  pages = {405--406},
  doi = {10.1017/s1743921317005658},
  url = {https://akademik.atauni.edu.tr/yayinlar/62225-searching-for-planets-around-eclipsing-binary-stars-using-timing-method-nsvs}
}