  Large-scale matter bulk flows with respect to the cosmic microwave background
have very recently been detected on scales 100 Mpc/h and 300 Mpc/h by using two
different techniques showing an excellent agreement in the motion direction.
However, the unexpectedly large measured amplitudes are difficult to understand
within the context of standard LCDM cosmology. In this work we show that the
existence of such a flow could be signaling the presence of moving dark energy
at the time when photons decoupled from matter. We also comment on the relation
between the direction of the CMB dipole and the preferred axis observed in the
quadrupole in this scenario.
