Formation and evolution of protostellar accretion discs - II. From 3D simulation to a simple semi-analytic model of Class 0/I discs

Physics & Astronomy

• accretion disks 100%
• simulation 36%
• magnetic diffusion 9%
• stellar cores 9%
• gravitational instability 8%
• magnetohydrodynamic simulation 8%
• braking 8%
• protostars 8%
• tracing 7%
• field strength 5%
• angular momentum 5%

Earth & Environmental Sciences

• accretion 89%
• simulation 42%
• magnetohydrodynamics 15%
• angular momentum 14%
• magnetic field 10%
• cooling 8%
• heating 8%
• young 8%
• modeling 5%