  We study holographic RG flows in a 3d supergravity model from the side of the
dynamical system theory. The gravity equations of motion are reduced to an
autonomous dynamical system. Then we find equilibrium points of the system and
analyze them for stability. We also restore asymptotic solutions near the
critical points. We find two types of solutions: with asymptotically AdS
metrics and hyperscaling violating metrics. We write down possible RG flows
between an unstable (saddle) UV fixed point and a stable (stable node) IR fixed
point. We also analyze bifurcations in the model.
