Bondi accretion, numerical hydrodynamic simulations
2017-07-28T20:37:32Z (GMT) by
Spherically symmetric hydrodynamical simulations of Bondi accretion, performed in two and three dimensions, using the PLUTO code.
These simulations reproduce the B1 and G3 cases of Ruffert et al. 1994 ApJ.
Part of MsC dissertation work of Henrique Gubolin, under the supervision of Prof. Rodrigo Nemmen.
• DBL datasets with grids, density, velocities and pressure fields
• initial and boundary condition information necessary to reproduce the simulations with Pluto
• movies showing the evolution of some fields