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Fig. 3.

image

Maps of v/σ for the stellar components in the TIMER galaxies, as indicated. The plotted range is indicated on the bottom right corner. The isophotes shown are derived from the MUSE data cube reconstructed intensities and are equally spaced in steps of about 0.5 mag. On average, 1″ corresponds to ≈100 pc. North is up, east to the left.

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