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Fig. 5

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[C ii] profile toward the peak of the Orion Bar emission (5h35m20.6s, −5°25′5′′) averaged over a 43′′ (FWHM) Gaussian beam representing the resolution of the previous KAO observations (solid line). The dotted spectrum represents the widely distributed emission as measured on our secondary OFF position 12.3′ away from the Orion Bar in a region without molecular emission. The dashed lines show Gaussian fits to the two profiles.

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