Thermal and fragmentation properties of star-forming clouds in low-metallicity environments

Earth and Planetary Sciences

• Metallicity 100%
• Fragment 100%
• Fragmentation 80%
• Core 60%
• Thermal Evolution 40%
• Mass Distribution 40%
• Cosmic Microwave Background Radiation 40%
• Cooling 40%
• Gas 40%
• Mass 40%
• Normal Density Functions 20%
• Perturbation Theory 20%
• Deuterium 20%
• Chemical Evolution 20%
• Elongation 20%
• Gas Temperature 20%
• Model 20%
• Investigation 20%
• Length 20%
• Temperature 20%
• Fraction 20%
• Environment 20%
• Balance 20%
• Assumption 20%
• Falling 20%
• Dust 20%

Physics

• Metallicity 100%
• Clouds 100%
• Fragmentation 80%
• Cores 60%
• Cooling 40%
• Mass Distribution 40%
• Clump 40%
• Stars 40%
• Gases 40%
• Mass 40%
• Deuterium 20%
• Perturbation Theory 20%
• Gas Temperature 20%
• Elongation 20%
• Initial Mass Function 20%
• Jeans Mass 20%
• Chemical Evolution 20%
• Temperature 20%
• Model 20%
• Fractions 20%
• Environment 20%
• Dust 20%