Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation (2021)
Attributed to:
Astronomy at Durham 2020-2023
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2105.04560
Publication URI: https://arxiv.org/abs/2105.04560
Type: Other