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Fig. A.3

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Azimuthal dependence of the local line profile, for direct comparison to the data in Fig. 5, obtained analytically through a simple combination of the Keplerian shear estimated in this section for HD 121617, the system’s parameters at r = 73 au, a broadened line profile for 12CO with a velocity width of ~ 800 m s−1, and our instrumental spectral response with a resolution of 26 m s−1.

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