Fig. 13
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Polarised-light Qϕ for λobs= 1.2 μm for TD20.While the layout of the rows (inclinations) and columns (models) is the same as for the scattered-light images, no artificial coronagraph is applied. The dotted white (black) line indicates the (τ = 1)-surface as seen from r = 0 (z = ∞). The wind produces a distinct signature especially around the jet region.
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