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Fig. 1.


Large-scale HI distribution of models with different cluster orbits and wind angles (30°, 45°, 60°), i.e. the angle between the ram-pressure wind and the galactic disk. The projection angles are i = 90° (edge-on) and PA = 90° (horizontal). The Lorentzian ram-pressure profiles with shorter widths have higher values of peak ram pressure. Contour levels are (3, 6, 9, 15, 30, 150) × 1019 cm−2. The times of interest are 240 Myr, 210 Myr, and 200 Myr after peak ram pressure for wind angles of 30°, 45°, and 60°, respectively.

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