吸积黑洞磁化喷流的广义相对论建模
高能天体物理现象
2015-06-04 v1 宇宙学与河外天体物理
广义相对论与量子宇宙学
摘要
近期在喷流的广义相对论磁流体力学建模方面的进展，为驱动活动星系核（AGN）及其他吸积系统中喷流的吸积黑洞的内部工作机制提供了前所未有的见解。我将介绍近期确定喷流功率自旋依赖性的研究结果，并讨论其对 AGN 射电噪/静二分性以及近期在若干 AGN 中观测到高喷流功率现象的启示。
引用
@article{arxiv.1202.2864,
title = {General Relativistic Modeling of Magnetized Jets from Accreting Black Holes},
author = {Alexander Tchekhovskoy and Jonathan C. McKinney and Ramesh Narayan},
journal= {arXiv preprint arXiv:1202.2864},
year = {2015}
}
备注
8 pages, 4 figures. For an associated movie, see http://youtu.be/nRGCNaWST5Q . To appear in the proceedings of the conference "The Central Kiloparsec in Galactic Nuclei: Astronomy at High Angular Resolution 2011", open access Journal of Physics: Conference Series (JPCS), published by IOP Publishing