Ambipolar diffusion and star formation: Formation and contraction of axisymmetric cloud cores. II. Results

Engineering

• Phase Dynamic 100%
• Axisymmetric 100%
• Magnetic Field Line 100%
• Magnetic Field 50%
• Dimensionless 50%
• Initial State 50%
• Initial Condition 50%
• Field Strength 50%
• Equilibrium State 50%
• Magnetic Flux 50%
• Field Line 50%
• Free Parameter 50%
• Free Fall 50%
• Reference State 50%
• Collision Time 50%

Keyphrases

• Quasi-static 100%
• Star Formation 100%
• Ambipolar Diffusion 100%
• Magnetic Field Lines 33%
• Dynamic Phase 33%
• Flux Ratio 33%
• Thermal Pressure 33%
• Magnetic Pressure 16%
• Cm(III) 16%
• Parameter-free 16%
• Large Reduction 16%
• Field Lines 16%
• Equilibrium State 16%
• Magnetic Flux 16%
• Strength Increase 16%
• Self-initiated 16%
• Field Strength 16%
• Ion Density 16%
• Ion Collisions 16%
• Evolution Equations 16%
• Free Fall 16%
• Neutral Density 16%
• Gravitational Collapse 16%
• Parameter Study 16%
• Molecular Clouds 16%
• Central Density 16%
• Protostars 16%
• Reference State 16%
• Collision Time 16%
• Central Magnetic Field 16%
• Flux Loss 16%
• Dynamic Contractions 16%
• Time Loss 16%