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Fig. 13

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Radiative transfer images in the H-band (λ = 1.6 μm) of simulation runs with photoevaporation (left most column), β = 105 (center left column), β = 104 (center right column) and a cold magnetic wind with β = 104 (right most column). The upper panels are based on dust grains with a = 0.1 μm whereas the lower panels demonstrate synthetic images with a = 1 μm. The object is modeled at a distance of 150 pc with a solar type star at an inclination of 20°.

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