The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way (2020)
Attributed to:
Durham DiRAC-2 petascale facility
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2005.02401
Publication URI: https://arxiv.org/abs/2005.02401
Type: Other