Fig. 3.
Spatial distribution of the stellar mass fractions of different stellar populations (younger than 2.3 Gyr) in the LMC disc. The stellar populations are defined based on their age (indicated in the lower-right corner of each panel); youngest to oldest from the top-left to the bottom-right panels. The mass fraction is normalised to the mass in each spatial bin, i.e. the sum of the fractions of all populations (including older than 2.3 Gyr) in each spatial bin is 1.
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