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Fig. 12.

image

1st row: sketches of the model families described in Sect. 7.2. We show in all cases a cross section. 2nd row: photometry of the companion along with the model photometry for model parameters. The legend gives information about the assumed companion mass, size of the considered dust grains, and circumplanetary disk inclination (in models a and c). 3rd row: same as the second row, but for degree of linear polarization. Colors and line styles represent the same models as in the previous row.

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