Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations (2020)

First Author: Pfeffer J

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/staa3109

Publication URI: http://dx.doi.org/10.1093/mnras/staa3109

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4