The influence of the Hall effect on the global stability of cool protostellar disks
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20042499/pdf
Reference15 articles.
1. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
2. Linear Analysis of the Hall Effect in Protostellar Disks
3. Dynamo-generated Turbulence and Large-Scale Magnetic Fields in a Keplerian Shear Flow
4. The Disk Accretion Rate for Dynamo-generated Turbulence
5. Layered Accretion in T Tauri Disks
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1. Hall instability: origin, properties and asymptotic theory for its tearing mode;Journal of Plasma Physics;2021-07-14
2. Growth of magnetorotational instability in circumstellar discs around class 0 protostars;Monthly Notices of the Royal Astronomical Society;2021-04-30
3. Stability of a force‐free Hall equilibrium and release of magnetic energy;Astronomische Nachrichten;2019-07
4. The rotation of discs around neutron stars: dependence on the Hall diffusion;Monthly Notices of the Royal Astronomical Society;2017-10-09
5. Double Hall instability: A catalyzer of magnetic energy release;Astronomy Letters;2017-09
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