CMF2IMF – The Origin of the Stellar Initial Mass Function

The stellar Initial Mass Function (IMF) is a fundamental observable that shapes our understanding of galaxy evolution, star formation, and planet formation. Despite its apparent universality, the physical origin of the IMF remains a central open question in astrophysics.

This workshop brings together observational, theoretical, and computational experts to explore the link between the Core Mass Function (CMF) and the resulting stellar mass distribution. Key topics include:
- The role of turbulence, magnetic fields, and microphysics in core formation
- The evolution of dense cores during gravitational collapse
- Mass accretion and loss through outflows
- The dependence of the IMF on environment, metallicity, and feedback
- The impact of next-generation facilities (JWST, ALMA WBSU, ELT) on our understanding

Held at the ESO Headquarters in Garching, Germany, the event fosters interdisciplinary discussion through invited talks, contributed presentations, and collaborative sessions. The format supports deep scientific exchange in a vibrant academic environment.

Participation is limited to ensure high-quality interaction. Housing assistance and partial cost reimbursement are available for external participants.