Image Details
Caption: Fig. 22.
Fraction of stars formed in the past 0–1 Gyr (﹩f_{1}﹩), 1–6 Gyr (f6), and 6–14 Gyr (f14) plotted vs. MB for both M81 Group (orange triangles) and Local Group (blue circles) galaxies. The gray dashed line represents a transition luminosity noted by Lee et al. (2007) based on Hα EW measurements.
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