Fig. 7.
Properties of the cool CGM clouds described by our best model. All the profiles are plotted with respect to the intrinsic distance from the central galaxies and the different colored lines represent the result for the sixteen different galaxies of the sample. Top left: velocity profiles of the cool clouds. Top right and bottom left: respectively masses and radii of the cool clouds. Bottom right: cool CGM cumulative mass profile, with the vertical dashed line representing the distance of 160 kpc.
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