CORDIS Project
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This project focuses on understanding star formation by analyzing filamentary structures in molecular clouds. It aims to unify statistical tools to characterize the physical processes that lead to the formation of dense cores and stars.
The omnipresence of filamentary structures inside nearby molecular clouds observed by the Herschel space observatory challenges our comprehension of the star formation process.
We now know that most of the cold dense cores appear to form within those filaments, which suggest a possible link between the characterisation of the filamentary structure of molecular clouds and the core mass function (CMF).
Physical processes such as turbulence, gravitational fragmentation and the influence of magnetic…
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