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Fig. 7.

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Maps from the modified power-law temperature distribution model from Togi & Smith (2016). Left: Power-law index n, with lower values indicating a stronger contribution from hotter gas. Center: Lower temperature Tl, contributing to H2 emission. Right: Warm H2 mass per pixel, with each pixel area being ≈161 pc2. White contours trace CO(2–1) emission from cooler molecular gas. The dashed gray line marks the jet axis.

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