Journal article
Cosmological Simulations of Galaxy Formation I: Star Formation, Feedback, Resolution and Matching the Tully--Fisher Relation (among other things)
Abstract
We used fully cosmological, high resolution N-body+SPH simulations to follow
the formation of disk galaxies with a rotational velocity between 140 and 280
Authors
Governato F; Stinson G; Wadsley J; Quinn T
Journal
, , ,
Publication Date
September 9, 2005
DOI
10.48550/arxiv.astro-ph/0509263