Lagrangian Matter Tracers: No Jet
Throughout the simulation, we seed "particles" to serve as tracers of Lagrangian fluid elements. Then we track where these particles move as we follow the evolution of the matter. We choose to seed and track the particles that originate in the disk after the black hole forms. The particles move outward with the shock-heated "wind outflow." There is no jet in this case.
 t/M=28855 |
 t/M=28932 |
 t/M=29012 |
 t/M=29088 |
