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Two New Planets from the Anglo‐Australian Planet Search

  • Authors: R. Paul Butler, C. G. Tinney, Geoffrey W. Marcy, Hugh R. A. Jones, Alan J. Penny, and Kevin Apps

Butler et al. 2001 The Astrophysical Journal 555 410.

  • Provider: AAS Journals

Caption: Fig. 7.

Doppler velocities for HD 134987 (G5 V). The solid line is a Keplerian orbital fit with a period of 264.6 days, a semiamplitude of 53.7 m s−1, and an eccentricity of 0.37, yielding a minimum (﹩M\mathrm{sin}\,i﹩) of 1.63 ﹩M_{\mathrm{J}\,}﹩ for the companion. The rms of the Keplerian fit is 2.7 m s−1. These results are consistent with Vogt et al. (2000).

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