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The mass fraction of halo stars contributed by the disruption of globular clusters in the E-MOSAICS simulations (2020)

First Author: Reina-Campos M

Attributed to: DiRAC 3 Operations funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa483

Publication URI: http://dx.doi.org/10.1093/mnras/staa483

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3