磁场对辐射冷却原恒星喷流结构的影响
天体物理学
2007-05-23 v1
摘要
本文利用完全三维光粒子磁子流体动力学 (SPMHD) 模拟，探讨磁场（与气体接近等分区）对辐射冷却、局部发达喷流结构及其对原恒星喷流动力学的影响。
引用
@article{arxiv.astro-ph/9808194,
title = {Magnetic Field Effects on the Structure of Radiatively Cooling Protostellar Jets},
author = {Elisabete M. de Gouveia Dal Pino and Adriano H. Cerqueira},
journal= {arXiv preprint arXiv:astro-ph/9808194},
year = {2007}
}
备注
4 pages; To appear in the proceedings of the 1998 International Conference on Plasma Physics, Praha (Czech Republic) 07/29-07/03/1998