Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations (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.2003.00076
Publication URI: https://arxiv.org/abs/2003.00076
Type: Other