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How gas flows shape the stellar-halo mass relation in the EAGLE simulation (2021)

First Author: Mitchell P

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