Magnetic Field Effects on the Structure of Radiatively Cooling Protostellar Jets

Preprint

19 August 1998

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/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.

Keywords

STRUCTURE OF RADIATIVELY
MAGNETIC FIELD EFFECTS
COOLING PROTOSTELLAR
RADIATIVELY COOLING
PROTOSTELLAR JETS
NONLINEAR EFFECTS

All Related Versions

Version 1, 1998-08-19, ArXiv

This publication has 0 references indexed in Scilit: