Magnetorotationally driven galactic turbulence and the formation of giant molecular clouds

Keyphrases

• Density Weight 20%
• Dimensionless Characteristics 20%
• Disc Compression 20%
• Flat Rotation Curves 20%
• Giant Molecular Clouds 100%
• High Amplitude 20%
• Jeans Mass 20%
• Magnetic Braking 20%
• Magnetorotational Instability 100%
• Maxwell Stress 20%
• Nonlinear Stability 20%
• Reynolds Stress 20%
• Saturated State 40%
• Self-gravitating Disk 20%
• Self-gravity 60%
• Shear-compression 20%
• Spin Angular Momentum 20%
• Spin Axis 20%
• Uniform Shear 20%

Physics

• Giant Molecular Clouds 100%
• Jeans Mass 33%