NUMERICAL SIMULATION OF THE XZ TAURI SUPERSONIC ASTROPHYSICAL JET

被引：0
|
作者：
Carl L. Gardner [1 ]
Steven J. Dwyer [1 ]
机构：
[1] School of Mathematical and Statistical Sciences, Arizona State University, Tempe AZ 85287, USA
来源：
ActaMathematicaScientia | 2009年 / 29卷 / 06期
关键词：
astrophysical jets; ENO method; gas dynamics;
D O I：
暂无
中图分类号：
P14 [天体物理学];
学科分类号：
070401 ;
摘要：
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.
引用
收藏
页码：1677 / 1683
页数：7
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