Fig. 9 from Two New Planets from the Anglo‐Australian Planet Search

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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. 9.

Phased Doppler velocities for HD 75289 (G0 V). The solid line is a Keplerian orbital fit with a period of 3.508 days, a semiamplitude of 56 m s⁻¹, and an eccentricity of 0.01, yielding a minimum (﹩M\mathrm{sin}\,i﹩) of 0.45 ﹩M_{\mathrm{J}\,}﹩ for the companion. The rms of the Keplerian fit is 4.8 m s⁻¹. These results are consistent with Udry et al. (2000).

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