Launching of accretion disc winds along dynamo-generated magnetic fields
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/310/4/1175/18634498/310-4-1175.pdf
Reference11 articles.
1. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
2. Hydromagnetic flows from accretion discs and the production of radio jets
3. Modelling magnetised accretion discs
4. The dependence of the dynamo alpha on vorticity
5. Dynamo-generated Turbulence and Large-Scale Magnetic Fields in a Keplerian Shear Flow
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1. Jets from Accretion Disk Dynamos: Consistent Quenching Modes for Dynamo and Resistivity;The Astrophysical Journal;2022-08-01
2. Magnetohydrodynamic Accretion–Ejection: Jets Launched by a Nonisotropic Accretion-disk Dynamo. I. Validation and Application of Selected Dynamo Tensorial Components;The Astrophysical Journal;2020-09-01
3. Self-gravity in magnetized accretion discs as a result of a dynamo mechanism with outflows;Monthly Notices of the Royal Astronomical Society;2020-02-29
4. Magnetic field amplification via protostellar disc dynamos;Monthly Notices of the Royal Astronomical Society;2018-03-08
5. Accretion Disc Magnetic Winds;Astrophysics and Space Science Library;2018
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