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.
initial conditions 2x512**3


Density map of a comobile cube (20Mpc^3/h^3) of the univers at z=6.

univers


Sterescopic view of the univers at z=0.
(blue: gas, green:dark matter, red:stars)

univers


Sterescopic zoom of a cluster in a cosmological simulation.
(blue: gas, green:dark matter, red:stars)

amas


Evolution of a makino univers.



Isolated and interacting galaxies

3D model of the MilkyWay warp

milkywaywarp


Bending instabilities in spiral galaxies
(edge-on density map, face-on density map, z map, araki ratio map)

bending


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

multiphase


Stereoscopic view of interacting galaxies


Sample of interacting galaxies
merger


Cluster of galaxies

Evolution of buoyantly plasma bubbles in a cooling flow cluster
(temperature map, density map, entropy map)

cluster


Temperature evolution of buoyantly plasma bubbles in a cooling flow cluster

cluster2


Formation of cold gas in a cooling flow cluser perturbed by plasma bubbles



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