Fig. 1
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HST (left) and MUSE (right) field images of the region around 244–440. The fields and insets in both images are shown in the [O I]λ6300 Å emission. The stars θ2 Orionis A and B are seen just below the proplyd to the southwest and southeast, respectively. The inset in the MUSE panel is a flux-integrated image from our current NFM observations discussed in Sect. 2.1.
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