Fig. 2.
Baryonic effect on the mean radial pairwise velocity as function of pair separation, at z = 0 for various hydrodynamical simulations. Top panel: ratio between the mean radial pairwise velocity of gas with that of the matter from collisionless simulation, while middle panel: ratio between the mean radial pairwise velocity of the dark matter from the full physics run to that of the collisionless simulation. Bottom panel: ratio between the matter from hydrodynamical and collisionless simulations.
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