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Fig. 14


Sketch of the proposed geometry of G202.3+2.5. The red structure corresponds to the main filament, the blue ones to the northern filaments. The front side of the main filament is illuminated by the cluster stars, and is responsible for most of the scattered light in the area 1 of Fig. 13. The northern filaments are in the shadow of material between them and the cluster, and are seen in extinction in front of background emission in the area 2 of Fig. 13.

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