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Planetary Companions to the Metal‐rich Stars BD −10°3166 and HD 52265

  • Authors: R. Paul Butler, Steven S. Vogt, Geoffrey W. Marcy, Debra A. Fischer, Gregory W. Henry, and Kevin Apps

Butler et al. 2000 The Astrophysical Journal 545 504.

  • Provider: AAS Journals

Caption: Fig. 4.

Phased Doppler velocities for BD −10°3166. The same best‐fit sinusoid is shown in Figs. 3 and 4. The rms to the sinusoidal fit is 8.1 m s﹩^{-1}﹩, slightly worse than the best‐fit Keplerian. The period is 3.487 days, and the semiamplitude is 60.6 m s﹩^{-1}﹩. Assuming the mass of BD −10°3166 is 1.1 M﹩_{\odot }﹩, the minimum (﹩M\mathrm{sin}\,i﹩) mass of the companion is 0.48 M﹩_{\mathrm{JUP}\,}﹩, and the semimajor axis is 0.046 AU.

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