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Fig. 9
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Results from the N-body ZLK migration simulations of HAT-P-26 b. Left to right : semimajor axis, ab, stellar obliquity, ψAb, mutual inclination, ψbB, between the orbits of planet b and companion B, and the orbital eccentricity, eb. Dashed and dotted black lines mark the observed values and 1σ uncertainties.
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