Fig. 20.
Variation of the stripped gas fraction within the tail in its different phases (black: HI; blue: H2; red: ionised) as a function of time for the simulated galaxy subject to an external wind of 2000 km s−1 (solid) and 1200 km s−1 (dashed). The black, blue, and red arrows on the Y-axis indicate for reference the mean HI, H2, and HII gas fractions on the leading side of the unperturbed galaxy disc.
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