CORDIS Project
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This project aims to develop a comprehensive understanding of star formation processes within molecular clouds. It combines large-scale simulations with detailed studies of protostellar formation to explore the interplay of various physical mechanisms involved in star birth.
New stars form within large turbulent complexes harboring several thousands of solar masses of cold gas: the molecular clouds.
The diffuse gas collapses gravitationally and heats up via compression until nuclear fusion reactions ignite and the star comes to life.
The full description involves an intricate interplay between large-scale environmental factors and small-scale processes close to the star, connecting a number of physical mechanisms, including magnetic fields, self-gravity, radiative t…
KOBENHAVNS UNIVERSITET
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