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Magnetohydrodynamic stability of broad line region clouds
Martin Krause
, M. Schartmann
, A. Burkert
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Research output
:
Contribution to journal
›
Article
›
peer-review
18
Citations (Scopus)
25
Downloads (Pure)
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Dive into the research topics of 'Magnetohydrodynamic stability of broad line region clouds'. Together they form a unique fingerprint.
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Keyphrases
Broad Line Region
100%
Magnetic Field
100%
Active Galactic nuclei
100%
Magnetohydrodynamic Stability
100%
Hydrodynamic Stability
50%
Gravitational Force
50%
Magnetic Configuration
50%
Cloud Stability
50%
Stationary Density
50%
Pressure Support
50%
Helical Magnetic Field
50%
Column Density
50%
Cloud Model
50%
Internal Motion
50%
Magnetic Field Configuration
50%
Kelvin-Helmholtz
50%
Magnetohydrodynamic Simulation
50%
Stability Properties
50%
Resolution Level
50%
Radiation Pressure
50%
Gauss
50%
Power Law
50%
Density Histogram
50%
Supermassive Black Holes (SMBHs)
50%
Thermal Pressure
50%
Azimuthal Magnetic Field
50%
Physics
Magnetohydrodynamic Stability
100%
Magnetic Field
100%
Active Galactic Nuclei
66%
Supermassive Black Holes
33%
Radiation Pressure
33%
Magnetic Field Configurations
33%
Magnetohydrodynamic Simulation
33%
Flow Stability
33%