Fig. 2.
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Stellar mass (top row) and mass-weighted age (bottom row) distributions of Hα (red histograms) and UV (blue histograms) clumps. The clumps were divided into tail (left panels) and extraplanar (right panels) according to the criteria described in Sect. 2.1, and the sample was selected following the procedure described in Sect. 2.3.
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