The SOPHIE search for northern extrasolar planets - X. Detection and characterization of giant planets by the dozen

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Fig. 11

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Evolution in the HIP 65407 two-planet system of the angle Δω = ω_c − ω_b (red line), which oscillates around 180° with a maximal amplitude of 45°. The green and black lines (nearly overplotted) also give the Δω evolution, but obtained with the linear secular models (Eqs. (1) and (2), respectively).

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