Persistent URL of this record https://hdl.handle.net/1887/3561356
Documents
-
- Download
- 2103.10966
- Accepted Manuscript
- open access
- Full text at publishers site
In Collections
This item can be found in the following collections:
How gas flows shape the stellar-halo mass relation in the EAGLE simulation
- All authors
- Mitchell, P.D.; Schaye, J
- Date
- 2022
- Volume
- 511
- Issue
- 2
- Pages
- 2948 - 2967