Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation (2020)
Attributed to:
DiRAC 2.5y Bridging Funding - UCL
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa620
Publication URI: http://dx.doi.org/10.1093/mnras/staa620
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3