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Fig. 4


Cumulative distributions of mass within various projected separations w from the density ridgeline. Top and bottom panels show the integral-shaped filament (ISF) and remaining region of Orion A (L1641) respectively. The cumulative distributions start at the southern boundary of each structure. The separate cumulative distributions for the east (− w<x< 0) are west (0 <x< + w) are shown in different line types. For ease of comparison (and clarity) these are multiplied by two.

This figure is made of several images, please see below:

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