How gas flows shape the stellar-halo mass relation in the EAGLE simulation (2021)
Attributed to:
DiRAC: Memory Intensive 2.5y
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2103.10966
Publication URI: https://arxiv.org/abs/2103.10966
Type: Other