Precise radial velocities of giant stars - XI. Two brown dwarfs in 6:1 mean motion resonance around the K giant star ν Ophiuchi

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Fig. 8

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As in Figs. 6 and 7, but for e₂ vs. ω₂. All fits on this grid are stable for at least 10 Myr, and the fits within the formal 3σ confidence level are in 6:1 MMR with θ₁–θ₆ librating around 0°. See text for details.

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