Structure of photodissociation fronts in star-forming regions revealed by Herschel observations of high-J CO emission lines

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Fig. 5.

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Line profile for the J = 10–9 transition of ¹²CO (dashed line) and ¹³CO (dotted line) in the Orion Bar (top panel) and NGC 7023 NW (bottom panel). The relative intensity of the ¹²CO to ¹³CO lines across the velocity profiles is also shown (plain line).

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