Primordial star formation under far-ultraviolet radiation

Physics

• Clouds 100%
• Population III Stars 100%
• Star Formation 100%
• Far Ultraviolet Radiation 100%
• Hydrogen 50%
• Cooling 50%
• Molecules 33%
• Emission 16%
• Fragmentation 16%
• Solar Mass 16%
• Collapse 16%
• Mass 16%
• Chemical Evolution 16%
• Jeans Mass 16%
• H1 Line Emission 16%
• Gaseous State 16%