Non-ideal magnetohydrodynamics versus turbulence - I. Which is the dominant process in protostellar disc formation? (2020)
Attributed to:
DiRAC 2.5y Bridging Funding - UCL
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