Magnetic Field Effects on the Structure of Radiatively Cooling Protostellar Jets
arXiv:astro-ph/9808194
Abstract
In the present work, with the help of fully 3-D smooth particle magnetohydodynamic (SPMHD) simulations, we explore the nonlinear effects of magnetic fields (in close equipartition with the gas) in the structure of radiatively cooling, overdense jets and test their importance on the dynamics of protostellar jets.
4 pages; To appear in the proceedings of the 1998 International Conference on Plasma Physics, Praha (Czech Republic) 07/29-07/03/1998