Preprint
The Dual Origin of Stellar Halos II: Chemical Abundances as Tracers of Formation History
Abstract
Fully cosmological, high resolution N-Body + SPH simulations are used to
investigate the chemical abundance trends of stars in simulated stellar halos
Authors
Zolotov A; Willman B; Brooks A; Governato F; Hogg DW; Shen S; Wadsley J
Publication date
April 21, 2010
DOI
10.48550/arxiv.1004.3789
Preprint server
arXiv