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

NASIROĞLU İ., GOZDZIEWSKI K., Slowikowska A., KRZESZOWSKİ K., ZEJMO M., Zola S., ...More

330th Symposium of the International-Astronomical-Union (IAU), Nice, France, 24 - 28 April 2017, vol.12, pp.405-406, (Full Text) identifier

  • Publication Type: Conference Paper / Full Text
  • Volume: 12
  • Doi Number: 10.1017/s1743921317005658
  • City: Nice
  • Country: France
  • Page Numbers: pp.405-406
  • Ataturk University Affiliated: Yes

Abstract

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.