  We have shown the simultaneous generation of macro-scale fast flows and
strong magnetic fields in the 2-temperature relativistic electron-ion plasmas
of astrophysical objects due to Unified Reverse Dynamo/Dynamo mechanism. The
resulting dynamical magnetic field amplification and/or flow acceleration is
directly proportional to the initial turbulent kinetic/magnetic (magnetic)
energy; the process is very sensitive to relativistically hot electron-ion
fraction temperature and magneto-fluid coupling. It is shown, that for
realistic physical parameters of White Dwarfs accreting hot astrophysical flow
/ Binary systems there always exists such a real solution of dispersion
relation for which the formation of dispersive strong super-Alfv\'enic
macro-scale flow/outflow with Alfv\'en Mach number $> 10^6$ and/or generation
of super-strong magnetic fields is guaranteed.
