CORDIS Project
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This project investigates the chemical evolution of interstellar matter, focusing on how elements transition from gas to solid forms in dense clouds. By modeling these processes, it aims to better understand the conditions for planet formation and the origins of complex molecules.
At the end of their life, stars spread their inner material into the diffuse interstellar medium.
This diffuse medium gets locally denser and form dark clouds (also called dense or molecular clouds) whose innermost part is shielded from the external UV field by the dust, allowing for molecules to grow and get more complex.
Gravitational collapse occurs inside these dense clouds, forming protostars and their surrounding disks, and eventually planetary systems like (or unlike) our solar system.
Th…
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
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