CORDIS Project
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This project aims to understand the mechanisms of mass ejection and jet formation in young stars through high-resolution observations. It utilizes advanced interferometric techniques to investigate the interplay between accretion and ejection processes in star formation.
A crucial problem in star formation is to understand the physical mechanism by which mass is ejected by young stars and collimated into stellar jets and the nature of the link with the accretion process.
The interaction of outflowing material with the parental cloud is observable on scales from hundreds of astronomical units (AU) up to parsec scales and is relatively well understood.
Conversely, both accretion and ejection take place on very small scales, from a few down to fractions of AU (i.e.…
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