Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation (2019)
Attributed to:
DiRAC-2.5 - the pathway to DiRAC Phase 3
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1905.01612
Publication URI: https://arxiv.org/abs/1905.01612
Type: Other