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A planetary companion orbiting the intermediate-mass G Giant HD 173416
Authors:Yu-Juan Liu  Bunei Sato  Gang Zhao  Hiroyasu Ando
Institution:[1]National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China [2]Tokyo Institute of Technology, 2-12-10okayama, Meguro-ku, Tokyo 152-8550, Japan [3]National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan [4]Deparfment of Astronomy, Graduate University for Advanced Studies, Shonan Village, Hayama, Kanagawa, 240-0193, Japan
Abstract:The discovery of a planetary companion to the intermediate-mass late-type giant star HD173416 from precise Doppler surveys of G and K giants at Xingiong station and Okayama Astrophysical Observatory (OAO) is presented in this letter. The planet has a minimum mass of 2.7 MJ an eccentricity of 0.21, a semimajor axis of 1.16 AU and an orbital period of 324 days.
Keywords:planetary systems-stars: individual: HD173416-stars: Planetary Systems-techniques: radial velocities
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