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Fig. 7.


Final Qϕ (left) and Uϕ (right) images of TW Hydrae. Qϕ and Uϕ are displayed with identical linear scale, and either unscaled (top) or scaled with r2 (bottom) to compensate for the decrease in stellar flux with distance. All four panels are shown with north up and east to the left for the same FoV of 4.9″ × 4.9″ or up to a separation of r = 2.45″ from the star in both RA (−x-axis) and Dec (+y-axis).

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