Spherically symmetric hydrodynamical simulations of Bondi accretion, performed in two and three dimensions, using the PLUTO code. <div><br></div><div>These simulations reproduce the B1 and G3 cases of Ruffert et al. 1994 ApJ.</div><div><br></div><div>Part of MsC dissertation work of Henrique Gubolin, under the supervision of Prof. Rodrigo Nemmen.</div><div><br></div><div>Included are:</div><div>• DBL datasets with grids, density, velocities and pressure fields</div><div>• initial and boundary condition information necessary to reproduce the simulations with Pluto</div><div>• movies showing the evolution of some fields</div
