CORDIS Project
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This project explores the formation of molecules in the early universe, focusing on turbulent dissipation in star-forming regions. It combines observational data with theoretical models to understand the dynamics of turbulence and its role in galaxy formation.
The discovery of molecules in the early universe is a challenging providence.
Molecules unveil the truly cold universe in which stars form and their rich versatility provides unique diagnostics to unravel the ”relative importance of purely gravitational effects and gas dynamical effects involving dissipation and radiative cooling”, recognized 40 years ago by White and Rees to be a central issue in theories of galaxy formation.
Molecules also reveal that cosmic turbulence is far less dissipative…
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