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A possible substellar companion to the intermediate-mass giant HD 175679
Authors:Liang Wang  Bun'ei Sato  Gang Zhao  Yu-Juan Liu  Kunio Noguchi  Hirovasu Ando  Hideyuki Izumiura  Eiji Kambe  Masashi Omiya  Hiroki Harakawa  Fan Liu  Xiao-Shu Wu  Yoichi Takeda  Michitoshi Yoshida  Eiichiro Kokubo
Institution:[1]Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China [2]Graduate University of Chinese Academy of Sciences, Beijing 100049, China [3]Department of Earth and Planetary Sciences, Graduate Sclaooi of Science and Engineering,Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan [4]National Astronomical Observatory of Japan, National Institutes of Natural Sciences,. Mitaka,Tokyo 181-8588, Japan [5]Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, NationalInstitutes of Natural Sciences, Asakuchi, Okayama 719-0232, Japan [6]Hiroshima Astrophysical Science Center, Hiroshima University, -1-3-1 Kagamiyama,Higashi-Hiroshima 739-8526, Japan
Abstract:
Keywords:stars: individual (HD 175679) -- stars: brown dwarfs -- techniques:radial velocities
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