  In this work we study oscillating soliton stars (oscillatons) with network of
domain walls. We consider a Lagrangian with three scalar fields coupled among
themselves by a specific potential. We choose an appropriate potential to admit
the formation of network of domain walls on the oscillatons. With small
perturbations applied to this potential, we then compute the
Einstein-Klein-Gordon (EKG) equations numerically and analyze the mass profile
of this new object. From the results we discuss how the stability of the
oscillatons is affected by the network. At some conditions the network provides
a `bouncing stability' to the oscillatons.
