Rigging dark haloes: why is hierarchical galaxy formation consistent with the inside-out build-up of thin discs?
State-of-the-art hydrodynamical simulations show that gas inflow through the virial sphere of dark matter haloes is focused (i.e. has a preferred inflow direction), consistent (i.e. its orientation is steady in time) and amplified (i.e. the amplitude of its advected specific angular momentum increas...
Main Authors: | Pichon, C, Pogosyan, D, Kimm, T, Slyz, A, Devriendt, J, Dubois, Y |
---|---|
Format: | Journal article |
Sprog: | English |
Udgivet: |
2011
|
Lignende værker
-
Rigging dark halos: why is hierarchical galaxy formation consistent with
the inside-out build-up of thin discs?
af: Pichon, C, et al.
Udgivet: (2011) -
Connecting the cosmic web to the spin of dark halos: implications for
galaxy formation
af: Codis, S, et al.
Udgivet: (2012) -
The angular momentum of baryons and dark matter halos revisited
af: Kimm, T, et al.
Udgivet: (2011) -
Inferring dark matter halo properties for H i-selected galaxies
af: Yasin, T, et al.
Udgivet: (2023) -
Swirling around filaments: are large-scale structure vortices spinning up dark haloes?
af: Laigle, C, et al.
Udgivet: (2014)