Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment (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.2110.03856
Publication URI: https://arxiv.org/abs/2110.03856
Type: Other