Fig. 11
Synthetic observations of the v5blb model at Δt ∈{0, 1, 2.5, 4, 6} × 4.4828 kyr after injecting the perturbation in 70 μm dust emission [Jy sr−1] at a distanceof 617 pc at different angles: with the LOS in the direction of the star’s relative motion (top) and at 45° to the ecliptic’s face-on view (bottom). The solid angle per pixel is 4.00 × 10−8 sr.
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