Cluster assembly and the origin of mass segregation in the STARFORGE simulations

Physics

• Molecular Cluster 100%
• Gases 60%
• Star Formation 40%
• Stars 30%
• Simulation 20%
• Shapes 20%
• Sites 20%
• Feedback 20%
• Magnetic Fields 10%
• Mass Distribution 10%
• Stellar Populations 10%
• Molecular Clouds 10%
• Be Type Star 10%
• Massive Stars 10%
• Expulsion 10%
• Low-Mass Star 10%
• Radiation Distribution 10%
• Turbulence 10%
• Environment 10%
• Geometry 10%
• Fractions 10%
• Differences 10%
• Clouds 10%
• Stopping 10%

INIS

• gases 60%
• stars 50%
• simulation 30%
• feedback 20%
• clouds 20%
• levels 10%
• radiations 10%
• surfaces 10%
• interactions 10%
• environment 10%
• populations 10%
• origin 10%
• geometry 10%
• magnetic fields 10%
• density 10%
• configuration 10%
• periodicity 10%
• segregation 10%
• star clusters 10%
• turbulence 10%
• mass distribution 10%