Angular momentum transfer to a Milky Way disk at high redshift
An Adaptive Mesh Refinement cosmological resimulation is analyzed in order to test whether filamentary flows of cold gas are responsible for the build-up of angular momentum within a Milky Way like disk at z>=3. A set of algorithms is presented that takes advantage of the high spatial resolut...
Autors principals: | Tillson, H, Devriendt, J, Slyz, A, Miller, L, Pichon, C |
---|---|
Format: | Journal article |
Publicat: |
2015
|
Ítems similars
-
Simulations of mass accretion onto dark matter haloes and angular momentum transfer to a Milky Way disk at high redshift
per: Tillson, H
Publicat: (2012) -
Feeding compact bulges and supermassive black holes with low
angular-momentum cosmic gas at high redshift
per: Dubois, Y, et al.
Publicat: (2012) -
Feeding compact bulges and supermassive black holes with low angular momentum cosmic gas at high redshift
per: Dubois, Y, et al.
Publicat: (2012) -
Satellite survival in highly resolved Milky Way class haloes
per: Geen, S, et al.
Publicat: (2012) -
The angular momentum of baryons and dark matter halos revisited
per: Kimm, T, et al.
Publicat: (2011)