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Fig. 7

image

Integral area-extinction relation for Perseus, i.e., the physical cloud area above a given extinction threshold as a function of that threshold. The solid black line shows the result for the entire field, while the solid gray line shows the same quantity for the Herschel regions. The dashed line shows again the same quantity, but for the 2MASS/NICEST data. The red line shows the slope of the power law .

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