Non-ideal magnetohydrodynamics versus turbulence II: Which is the dominant process in stellar core formation? (2020)

First Author: Wurster J

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/staa1340

Publication URI: http://dx.doi.org/10.1093/mnras/staa1340

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4