Preprint
The Properties of Prestellar Discs in Isolated and Multiple Prestellar Systems
Abstract
We present high-resolution 3D smoothed particle hydrodynamics simulations of
the formation and evolution of protostellar discs in a turbulent molecular
Authors
Hayfield T; Mayer L; Wadsley J; Boley AC
Publication date
March 12, 2010
DOI
10.48550/arxiv.1003.2594
Preprint server
arXiv