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Fig. A.1


Light travel time spiral solutions from Eq. (10), originating at a shadowing clump at rrim = 0.1 au around a 1.5 M star. The panels show different inclinations – left panel: i = 0° (movie 1), middle panel: 30° (movie 2), right panel: 60° (movie 3). The instantaneous orbital phase of the video snapshots is πrad.

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