Preprint
Angular momentum transport and disk morphology in SPH simulations of galaxy formation
Abstract
We perform controlled N-Body/SPH simulations of disk galaxy formation by
cooling a rotating gaseous mass distribution inside equilibrium cuspy spherical
Authors
Kaufmann T; Mayer L; Wadsley J; Stadel J; Moore B
Publication date
January 6, 2006
DOI
10.48550/arxiv.astro-ph/0601115
Preprint server
arXiv