| 66 | [[Image(CFvelocity.png, 40%)]] |
| 67 | |
| 68 | These curves are the velocity of a given shell (i.e. the outer radius of the various concentric spheres that make up the ambient medium). If that is confusing, [https://astrobear.pas.rochester.edu/trac/wiki/u/erica/UniformCollapse see this page]. |
| 69 | |
| 70 | Here is the density of the sphere over time as it collapses (the density is increasing everywhere in the sphere at the same rate, hence the sphere continues to have a uniform density over time): |
| 71 | |
| 72 | [[Image(CFdensity.png, 40%)]] |
| 73 | |
| 74 | With these last two data sets, here are ram pressure radial profiles. Now the different curves represent time, and are only plotted from t = 0 to t = tsim: |
| 75 | |
| 76 | [[Image(CFrampressure.png, 40%)]] |
| 77 | |
| 78 | Now, the post shock density is comparable to the density of the infalling ambient. However, the velocity is very different, as it should be in retrospect. This leads to large deviations between the ram pressure of the infalling ambient and the ram pressure of the splashed material. |
| 79 | |
| 80 | The incoming flows have a high speed, and once shocked, though decreased, is still high. The ambient, however, is starting from rest. This means, that by the time the entire simulation has completed (i.e. long after the ring has formed), the ambient has still not acquired enough momentum to make the ram pressures balance. |
| 81 | |
| 82 | In hindsight, this was always going to be the case, as the ring is not present in the hydro case, and so the ambient's own dynamics are too weak to constrain outflowing material from the collision region. |