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