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Fig. 10.

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Surface mass density of the stellar component for a galaxy from the IllustrisTNG simulations with a stellar mass and rotational velocity similar to those of the Milky Way (ID 486966). Left panel: Face-on view of the galaxy. Right panel: Edge-on view of the galaxy. In both cases, the presence of a disk and spheroid component is evident at first glance. The color scale corresponds to surface stellar mass density.

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