Fig. 21.
Variation of the star formation rate within the whole galaxy (upper left panel), the front region (upper right), the leading side (lower left), and the tail of stripped gas (lower right) as a function of time for the simulated galaxy subject to an external wind of 2000 km s−1 (solid red) and 1200 km s−1 (dashed red) compared to an unperturbed system (dotted black).
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