| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 4664920 | Acta Mathematica Scientia | 2009 | 7 Pages |
Abstract
Computational gas dynamical simulations using the WENO-LF method are applied to modeling the high Mach number astrophysical jet XZ Tauri, including the effects of radiative cooling. Mach 55 simulations of the pulsed proto-jet are presented and analyzed in terms of interacting nonlinear waves: terminal Mach disks, bow shocks, and Meshkov-Richtmyer instabilities of the leading jet contact boundary.
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Physical Sciences and Engineering
Mathematics
Mathematics (General)
