Angular momentum transfer to a Milky Way disk at high redshift

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...

Bibliografski detalji
Glavni autori:	Tillson, H, Devriendt, J, Slyz, A, Miller, L, Pichon, C
Format:	Journal article
Izdano:	2015

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