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°.