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.
Original language | English (US) |
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Pages (from-to) | 1677-1683 |
Number of pages | 7 |
Journal | Acta Mathematica Scientia |
Volume | 29 |
Issue number | 6 |
DOIs | |
State | Published - Nov 2009 |
Keywords
- 65M06
- 76E20
- 76N15
- ENO method
- astrophysical jets
- gas dynamics
ASJC Scopus subject areas
- Mathematics(all)
- Physics and Astronomy(all)