Long-period Jovian planets at HD 86950 and HD 222076

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Long-period Jovian planets at HD 86950 and HD 222076

Post by Sirius_Alpha on 24th November 2016, 12:09 am

The Pan-Pacific Planet Search VI: Giant planets orbiting HD 86950 and HD 222076

We report the detection of two new planets orbiting the K giants HD 86950 and HD 222076, based on precise radial velocities obtained with three instruments: AAT/UCLES, FEROS, and CHIRON. HD 86950b has a period of 127057 days at a=2.720.08 AU, and m sin i=3.60.7 Mjup. HD 222076b has P=87119 days at a=1.830.03 AU, and m sin i=1.560.11 Mjup. These two giant planets are typical of the population of planets known to orbit evolved stars. In addition, we find a high-amplitude periodic velocity signal (K∼50 m/s) in HD 29399, and show that it is due to stellar variability rather than Keplerian reflex motion. We also investigate the relation between planet occurrence and host-star metallicity for the 164-star Pan-Pacific Planet Search sample of evolved stars. In spite of the small sample of PPPS detections, we confirm the trend of increasing planet occurrence as a function of metallicity found by other studies of planets orbiting evolved stars.

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