Fig. 15
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Sensitivity study on the mass and orbital period of a body causing the observed apsidal motion rate of ≃0.1727º d−1 by varying its orbital eccentricity and mass, according to Borkovits et al. (2011). The two grey shaded regions represent the same areas in Figure 14 (see text for more details). The vertical dashed line represents the orbital period of WASP-43b.
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