抗性磁性原行星喷流的发射
天体物理学
2007-05-23 v1
摘要
湍流吸积盘是原行星星体喷流最可能的来源。我们使用在轴对称选项中扩展的ZEUS-3D代码，来调查盘风向向准直喷流的演化。随着磁化扩散率的增加，抗性喷流传播得更慢，准直程度降低。包含抗性盘的模拟会喷射持续且高度准直的喷流。
引用
@article{arxiv.astro-ph/0311057,
title = {Launching of resistive magnetic protostellar jets},
author = {Miljenko Cemeljic and Christian Fendt},
journal= {arXiv preprint arXiv:astro-ph/0311057},
year = {2007}
}
备注
To appear in: Stars as Suns: Activity, Evolution and Planets, eds. A. K. Dupree, A. Benz, IAU Symposium no. 219 Proceedings