What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies (2021)
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.2101.08282
Publication URI: https://arxiv.org/abs/2101.08282
Type: Other