CORDIS Project
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This project utilizes advanced interferometric techniques to study the inner regions of protoplanetary discs around solar-like stars. It aims to enhance our understanding of planetary formation processes and disc dynamics.
A first step towards understanding planetary formation is the characterisation of the structure and evolution of protoplanetary discs.
Although the large scale disc is understood in some detail, very little is known about the inner 5 au (i.e. within a radius corresponding to Jupiter's orbit) in which the main physical processes take place: accretion, ejection and planetary formation.
For the nearest sites of star formation, this region is inaccessible to standalone telescopes, and only recently…
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