Baryonic Tully-Fisher relation of simulated dwarf galaxies, run with (left panel) and without (right panel) the inclusion of BH and AGN feedback. Each galaxy’s baryonic mass is measured within the virial radius and shown in a different colour according to its z = 0 BH mass, as in Fig. 3. Different symbols indicate different ways of measuring the rotational velocity, V_rot: V_DM, max, V_flat, and V_8h are shown as squares, triangles, and diamonds, respectively. The observational relations given by McGaugh (2012), are depicted with the solid line, and the relation obtained in Di Cintio & Lelli (2016) using semi-analytic models with the dotted line. Simulated galaxies that include AGN feedback are in better agreement with the observed BTFR.