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Sub‐Saturn Planetary Candidates of HD 16141 and HD 46375

  • Authors: Geoffrey W. Marcy, R. Paul Butler, and Steven S. Vogt

Marcy, Butler, & Vogt 2000 The Astrophysical Journal Letters 536 L43.

  • Provider: AAS Journals

Caption: Fig. 4.

Phased Doppler velocities for HD 46375. The same best‐fit sinusoid is shown in Fig. 3. The rms to the sinusoidal fit is 2.59 m s﹩^{-1}﹩, which is essentially identical to the best‐fit Keplerian. The period is 3.024 days, and the semiamplitude is 35 m s﹩^{-1}﹩. Assuming that the mass of HD 46375 is 1 M﹩_{\odot }﹩, the minimum (﹩M\mathrm{sin}\,i﹩) mass of the companion is 0.25 MJUP, and the semimajor axis is 0.041 AU.

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