63 | | In the matched ambient case, however, Pram>Pcrit only after t~2.3 myrs. By t =3 myrs, the Pram profile has taken on a very unique "cowboy-hat" appearance. Another look at the radial velocity plots and the density plots show that this is due to the high increase in density inside of the sphere by t=3myrs with small concomitant radial velocities, while outside of the sphere there are small density buildups coinciding with a large vrad, which when squared for Pram gives a large Pram outside as well. |
| 63 | In the matched ambient case, however, Pram>Pcrit only after t~2.3 myrs. By t =3 myrs, the Pram profile has taken on a very unique "cowboy-hat" appearance. Another look at the radial velocity plots and the density plots show that this is due to the high increase in density inside of the sphere by t=3myrs with small concomitant radial velocities, while outside of the sphere there are small density buildups coinciding with a large negative vrad, which when squared for Pram gives a large Pram outside as well. |