General Relativistic Magnetohydrodynamic Simulations of Jets from Black Hole Accretion Disks: Two-Component Jets Driven by Nonsteady Accretion of Magnetized Disks-Reference-Cited by-同舟云学术

General Relativistic Magnetohydrodynamic Simulations of Jets from Black Hole Accretion Disks: Two-Component Jets Driven by Nonsteady Accretion of Magnetized Disks

Published:1998-03-01 Issue:1 Volume:495 Page:L63-L66
ISSN:0004-637X
Container-title:The Astrophysical Journal
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Author:

Koide Shinji,Shibata Kazunari,Kudoh Takahiro

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference40 articles.

1. Abramowicz, M. 1996, in Physics of Accretion Disks, ed. S. Kato et al. (Amsterdam: Overseas Publishers Association), 1

2. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution

3. Asymptotic domination of cold relativistic MHD winds by kinetic energy flux

4. Hydromagnetic flows from accretion discs and the production of radio jets

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