Fig. A.1.
Two examples of massive (central) disc galaxies from the EAGLE simulations (run Ref-L0100N1504). The left and central panels show the systems from a face- and edge-on perspective. The right panels show the total circular velocity profiles (solid black lines), along with the separate contributions (dashed lines) from stars (orange), gas (blue), and dark matter (magenta). The vertical arrow shows the half-M⋆ radius.
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