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Fig. 4.

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Time required to assemble 80% of the ever-formed stellar mass of bulges and disks vs. the total present-day galaxy mass. Linear relations for both stellar components are over-plotted (solid lines for the bulge, dashed lines for the disk). The marks are colour coded according to their ⟨δμ9G⟩ interval (iA blue, iB green, iC red) and their size represents the measurements for bulge and disk (bigger and smaller circles, respectively).

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