Gallery¶
Cosmological simulations¶
Density map of a comobile cube (20Mpc^3/h^3) of the univers at z=40. 268 millions of particles have been used to create this map.
Density map of a comobile cube (20Mpc^3/h^3) of the univers at z=6.
Sterescopic view of the univers at z=0. (blue: gas, green:dark matter, red:stars)
Sterescopic zoom of a cluster in a cosmological simulation. (blue: gas, green:dark matter, red:stars)
Evolution of a makino univers.
Isolated and interacting galaxies¶
3D model of the MilkyWay warp
Bending instabilities in spiral galaxies (edge-on density map, face-on density map, z map, araki ratio map)
Winding of the line of node of a warped disk (z map, edge-on density map)
Velocity map of disks subjet to the bending instabilities
Edge on and Face on surface density maps of an evolving spiral galaxy
Edge on and Face on surface density maps with contours of a spiral galaxy
Edge on and Face on surface density maps with contours of a spiral galaxy
Stereoscopic view of interacting galaxies
Sample of interacting galaxies
Sample of interacting galaxies
Cluster of galaxies¶
Evolution of buoyantly plasma bubbles in a cooling flow cluster (temperature map, density map, entropy map)
Temperature evolution of buoyantly plasma bubbles in a cooling flow cluster
Formation of cold gas in a cooling flow cluser perturbed by plasma bubbles