Joel E. Tohline
John E. Cazes
Howard S. Cohl
Department of Physics & Astronomy
Louisiana State University
1. Astronomy Background
2. Summary of Research
Figure 1 |
Figure 2 |
3. Computational Tools
4. Example Simulations
MOVIE
Spiral-Mode Instability |
24-bit Quicktime format (2,554K) |
MOVIE
Velocity flow-Field in the Bar |
mpeg (2,421K) |
MOVIE "Massless" Torus |
MOVIE Self-Gravitating Torus |
Quicktime format (834K) 24-bit mpeg format (515K) |
mpeg format (190K) |
MOVIE Stable Binary |
MOVIE Binary Merger |
Quicktime format (834K) |
mpeg format (701K) |
5. High Peformance Fortran (HPF) and High-Performance-Computing
6. What Next?
7. Acknowledgments