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Fig. 3

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3.3 μm PAH intensity as a function of various stellar and disk parameters. From left to right are shown the parameter χ (FUV radiation field at 150 au from the star) and the FUV radiation field at the inner disk edge Rin and at the disk outer edge Rsize. The rightmost panel shows the 3.3 μm PAH intensity as a function of the total disk dust mass. Upper limits are indicated as empty circles with arrows. The Pearson correlation coefficient is indicated in the lower left corner of each panel.

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