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Fig. 10.

image

Perimeter-area relation (panel a) and cumulative size histogram (panel b) for the young stellar structures detected in the density map. The vertical dashed lines indicate the resolution limit of the KDE map and solid line are the best fits following the behavior of large structures. Fractal dimension values obtained in each case are indicated. Panel a: dashed sloped line shows the relation for a circle (P ∝ A0.5). Panel b: errors are from .

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