Fig. 10.
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Temporal evolution of the total baryonic mass enclosed within 500 pc from the centre of the two simulated dwarfs. The solid lines correspond to Bashful (red) and Doc (blue) in our simulation, with the superbubble feedback model. With the same colour convention, the same two dwarfs analysed in Shen et al. (2014) and Madau et al. (2014) are represented with dashed lines.
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