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Fig. 4


Stellar mass and line-of-sight orbital distribution of the simulated merger remnants M0-3 (the B/T ratio of their progenitors increases from left to right). The projected plane x-y corresponds to the orbital plane of the merger. From top to bottom: mass distribution log Σ, V, and σ. The CALIFA-like hexagonal field of view for the assumed distance is overplotted on the mock images of the first row.

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