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The mass fraction of halo stars contributed by the disruption of globular clusters in the E-MOSAICS simulations (2019)

First Author: Reina-Campos M

Attributed to: The Virgo consortium for cosmological supercomputer simulations funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1910.06973

Publication URI: https://arxiv.org/abs/1910.06973

Type: Other