Planetary Companions to the Metal-rich Stars BD –10°3166 and HD 52265*

@article{Butler2000PlanetaryCT,
  title={Planetary Companions to the Metal-rich Stars BD –10°3166 and HD 52265*},
  author={R. Paul Butler and Steven S. Vogt and Geoffrey W. Marcy and Debra A. Fischer and Gregory W. Henry and Kevin Apps},
  journal={The Astrophysical Journal},
  year={2000},
  volume={545},
  pages={504-511}
}
Precise Doppler measurements from the Keck/HIRES spectrometer reveal periodic Keplerian velocity variations in the stars BD -10°3166 and HD 52265. BD -10°3166 (K0 V) has a period of 3.487 days and a semiamplitude of 61 m s-1. An orbital fit yields a companion mass M sin i = 0.48 MJUP, a semimajor axis of a = 0.046 AU, and an eccentricity of e = 0.05 (consistent with zero). HD 52265 (G0 V) has a period of 119.0 days, a semiamplitude of 45 m s-1, an eccentricity of 0.29, a semimajor axis of a = 0… Expand
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