Left: mass models of NGC 7052. The X-ray derived dynamical mass (filled circles with error bars) is modeled (thin black line) including a stellar spheroid (dotted line) and a Burkert halo (dashed line). Also shown is the best-fit solution for the total mass for models that assume a NFW profile to represent the dark halo (blue line) or the MOND framework (red solid lines). r_e corresponds to 7.7 kpc. Right: mass models of NGC 7785. r_e corresponds to 5.6 kpc (see color figure online).