Fig. 8

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Dark matter spiral arms in other simulations. Sgr-NBody (upper two groups of panels): stellar density (first column), DM density (second column), ⟨VR⟩ (third column), and ⟨Vϕ⟩ (fourth column) after the second and third passages of a Sgr-like perturber (first and second rows, respectively). Hydro (bottom left group): stellar and DM density for two snapshots with strong spiral arms. Au27 (bottom right group): stellar and DM density for the last two snapshots in the simulation, z = 0 and z = 0.023.
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