- Barred galaxies
N-body simulation of barred galaxy
Face-on This simulation shows the evolution of a barred spiral galaxy. Only stars are shown, and colors represent their density. The dark matter halo is also present in the calculations, but not displayed in this animation.
N-body simulation of barred galaxy (almost edge-on)
Edge-on (almost) When the same galaxy is viewed under an inclination angle, one may notice the vertical thickness of the peanut-shaped bulge.
N-body simulation of barred galaxy (disk and halo)
Stellar disk and dark matter halo In this animation we see the evolution of a barred galaxy (in blue), but also of its dark matter halo (in orange). Both are seen face-on and edge-on. As the bar develops, the initially flattened halo becomes more spherical. For details, see the paper Machado & Athanassoula (2010).
N-body simulation of barred galaxy (slow)
Slowly rotating This animation shows the stellar disk of a simulated barred galaxy. Displaying more frequent time steps provides a better glimpse of the orbital structure.
-
Cluster mergers
Simulation of galaxy cluster merger: Abell 3376
Abell 3376 A comet-shaped cluster merger (gas density is shown)
Abell 2052 sloshing simulation: X-ray emission (model B)
Abell 2052 A sloshing cluster (X-rays)
Abell 2052 sloshing simulation: temperature (model B)
Abell 2052 A sloshing cluster (temperature)
Abell 1758 galaxy cluster merger simulation: X-ray emission
Abell 1758 A dissociative cluster (X-rays)
Abell 1758 galaxy cluster merger simulation: temperature
Abell 1758 A dissociative cluster (temperature)