Fig. 2.

Logarithm of total stellar mass ℳ⋆, T (M⊙) vs. radial age gradient within the bulge radius RB in Gyr/RB, as obtained from mass- and light-weighted stellar age determinations (∇(t⋆, B)ℳ and ∇(t⋆, B)ℒ; upper and lower panel, respectively). Symbols are color-coded according to the bulge classification scheme by BP18 (blue, green and red for iA, iB and iC bulges, respectively). Semi-transparent and solid markers correspond, respectively, to determinations from non-weighted and weighted linear fits. Bulges classified by BP18 as LINER (+) and Seyfert (x) are indicated. Dashed-dotted lines show non-weighted linear fits to weighted ∇(t⋆, B)ℳ and ∇(t⋆, B)ℒ determinations, the arithmetic average of which for the three bulge classes is depicted by stars.
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