Avancerad sökning
Hittade 2 avhandlingar som matchar ovanstående sökkriterier.
1. Chemodynamical Simulations of Star-Forming Molecular Clouds
Sammanfattning : Stars are known to form from dense, dusty clumps and cores of molecular clouds. However, there is no consensus on a theory that can predict the rate of star formation, its clustering, and the conditions needed for massive stars to be born. A major challenge is how to observe and characterise the gas that is the fuel for star formation. LÄS MER
2. Chemodynamics in Star-Forming Molecular Clouds
Sammanfattning : Stars are fundamental building blocks of galaxies. However, the answers to many basic questions about their formation remain elusive. There is no consensus on a theory that can predict the rate of star formation, its clustering properties, and the conditions needed for massive stars to be born. LÄS MER
