The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation (2018)

First Author: Kulier A
Attributed to:  Durham DiRAC-2 petascale facility funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1805.05349

Publication URI: https://arxiv.org/abs/1805.05349

Type: Other