The role of supernova feedback on the origin of the stellar and baryonic
  Tully-Fisher relations
  In this work, we studied the stellar and baryonic Tully-Fisher relations by
using hydrodynamical simulations in a cosmological framework. We found that
supernova feedback plays an important role on shaping the stellar Tully-Fisher
relation causing a steepening of its slope at the low-mass end, consistently
with observations. The bend of the relation occurs at a characteristic velocity
of approximately 100 km/s, in concordance with previous observational and
theoretical findings. With respect to the baryonic Tully-Fisher relation, the
model predicts a linear trend at z~0 with a weaker tendency for a bend at
higher redshifts. In our simulations, this behaviour is a consequence of the
more efficient action of supernova feedback at regulating the star formation
process in smaller galaxies.
