Fig. 6.

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Voronoi maps showing the 3D Jeans model fit to the LMC rotation field from the Gaia DR3 kinematic data. The first column represents the data in the X, Y, and LOS directions, respectively. Each Voronoi bin is colour-coded according to the median velocity of all stars that fall into it. The second column represents the Jeans model results and the third column the model residuals. PMs are converted into linear velocities. The velocity scale is kept unchanged between all maps for consistency and easier comparison.
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