Do we need non-ideal magnetohydrodynamics to model protostellar discs? (2021)
Attributed to:
DiRAC 2.5 Operations 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2101.04129
Publication URI: https://arxiv.org/abs/2101.04129
Type: Other