Preprint
The Role of Turbulence and Magnetic Fields in Simulated Filamentary Structure
Abstract
We use numerical simulations of turbulent cluster-forming regions to study
the nature of dense filamentary structures in star formation. Using four
Authors
Kirk H; Pudritz R; Klassen M; Pillsworth S
Publication date
January 23, 2015
DOI
10.48550/arxiv.1501.05999
Preprint server
arXiv