Non-ideal magnetohydrodynamics versus turbulence - I. Which is the dominant process in protostellar disc formation? (2020)

First Author: Wurster J
Attributed to:  DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission] funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa1339

Publication URI: http://dx.doi.org/10.1093/mnras/staa1339

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4