Fig. 12
R–t diagrams showing the radially averaged
distribution of light, mass, and SFR as a function distance from the nucleus and
age. Left: luminosity at λ = 5635 Å per unit area.
(ℒR,t). Middle: stellar mass formed
per unit area 
. Right:
time-dependent SFR per unit area 
.
The solid (white) lines represent the sum over all spaxels for a given age.
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