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Fig. 3

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Squared visibility and differential phases for the Be star reference model (Sect. 2) at radial velocities of vel. = −126 km s-1 and vel. = −200 km s-1 as a function of νobs, the ratio between the length of the baseline, and the distance of the target. The linear correspondence of the phase with the increasing spatial resolution (νobs ≲ 1.5 m pc-1) characterizes the astrometric regime.

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