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Fig. 4.


Ratio between the mean pairwise velocity of gas component with respect to collisionless matter at z = 0 for various runs in the cosmo-OWLS suite of simulations. The dotted line refers to the results from the “NoAGN” simulation, which had the AGN feedback switched off. While the dashed double-dotted line (“NoCool, UVB”) refers to the simulation that had no radiative cooling, star formation, or AGN feedback. There is, however, a net photo-heating due to a UV background.

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