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Fig. C.3

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Subarcsecond resolution RGB images of the Bar. Green represents the NIRCam F470M–F480M image (a proxy of the H2 v = 0–0 S (9) emission) and blue represents the C2H N = 4–3, F = 5–4 and F = 4–3 emission observed with ALMA. From left to right, red represents C18O J = 3–2 and [C I] 609 μm observed with ALMA, and JWST/NIRCam F335M–F330M image (PAH emission), respectively. We rotated the original images by 37.5 clockwise to bring the FUV illumination from the Trapezium in the horizontal direction (from the right).

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