Assessing the robustness of the Galactic rotation curve inferred from the Jeans equations using Gaia DR3 and cosmological simulations

Open Access

Fig. 10

Radial profiles of the three second moments of the velocity distribution in simulation L2 from Laporte et al. (2018). The top row shows t_{1,2,3,4,5}. The bottom row shows t₆ for both sides of the disc in x ≶ 0 and vertical cuts in ɀ ≶ 0, along with the equilibrium situation at t₁ for reference.

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