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Fig. 1

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RGB images (insets) of continuum subtracted, single line integrated flux images of the sample acquired with MUSE. In each inset, a variety of emission lines are combined to highlight the morphology of the proplyd. The background image is a Hubble optical image of the Orion Nebula Cluster (Credit: NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team).

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