Fig. 12

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H-band radial optical depth τobs originating from the central star depending on the inclination expressed in latitude for three dust species with sizes 0.1 μm, 1 μm and 10 μm indicated by the color scheme. The continuous lines refer to the photoevaporation simulation phc2, the dashed lines to the magnetic wind b5c2 with β = 105 and the dotted lines to the run b4c2 with β = 104.
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