Connecting the cosmic web to the spin of dark halos: implication for galaxy formation

by S. Codis, C. Pichon, J. Devriendt, A. Slyz, D. Pogosyan, Y. Dubois, T. Sousbie,

by C. Laigle, C. Pichon, S. Codis, Y. Dubois, D. Le Borgne, D. Pogosyan, J. Devriendt, S. Peirani, S. Prunet, S. Rouberol, A. Slyz, T. Sousbie,

by S. Codis, C. Pichon, D. Pogosyan,

The cosmic web of the the gas which end up in the bulge: intermediate time	The cosmic web of the the gas which end up in the bulge: late time	travelling of the inner region
walls of potential and velocity	spin relative to filament	walls wind up around each other to form a spinning structure along the filament	Time line of tracer particles of the gas
The vorticity flow arouud the main filament	The cross section of walls perpendicular to filament with vorticity vectors and velocity flow	the velocity flow and density of LSS	velocity field lines skeleton halos near main filament