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

IAU Symposium Proceedings Series(2018)

引用 0|浏览26
暂无评分
摘要
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.
更多
查看译文
关键词
binaries: eclipsing,ephemerides,planetary systems,NSVS14256825
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要