Context: Many objects that stellar and extragalactic astronomy study fall
into the category of accretion ejection systems. In the last years numerical
simulations have focused their interest in such systems, probing into
their mechanisms in an attempt to better comprehend the underlying
physics.

Aims:  In this work we study the effects of magnetization and anisotropic
diffusion on a sub-keplerian resistive accretion disk driving an ideal,
magnetised outflow. Issues like ejection efficiency, angular momentum and
energy transport, stability and the system's ability to reach an enduring
steady state are addressed.

Methods: With these in mind, we present a series of 2.5D axisymmetric MHD
simulations performed using the finite volume, shock capturing code,
PLUTO.

Results: We obtain the expected solutions for magnetization near  
equipartition. The extreme cases with either strong or weak magnetic field
configuration prove deficient in various aspects which are displayed. Also
the accretion-ejection dynamics for all configurations are discussed.