100 | | Finally, we have lineout movies of [attachment:press_lineout.gif pressure], [attachment:rho_lineout.gif density], and [attachment:vrad_lineout.gif vrad]. As these movies show, the Bondi solution is unaltered beyond $r>20$, as to be expected from the boundary conditions of the sim. Surprisingly, however, is that despite the density falling below its initial value in the kernel (due to accretion), the pressure spikes there seemingly artificially (rather than due to a build of material in the kernel). |
| 100 | Finally, we have lineout movies of [attachment:press_lineout.gif pressure], [attachment:rho_lineout.gif density], and [attachment:vrad_lineout.gif vrad]. As these movies show, the Bondi solution is unaltered beyond $r>20$, as to be expected from the boundary conditions of the sim. Surprising, however, is that despite the density falling below its initial value in the kernel (due to accretion), the pressure spikes there seemingly artificially (rather than due to a build of material in the kernel). |