CORDIS Project
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This project investigates the mechanisms behind jet formation in young stars, specifically classical T Tauri stars. By using advanced imaging techniques, it aims to provide observational data that will enhance understanding of how these jets are launched and their relationship with surrounding material.
The phenomenon of mass outflow from young stellar objects is arguably the most spectacular stage in the formation of a star.
Much is known of the large-scale manifestations of outflows and of their interactions with their parent molecular clouds.
However, in comparison, little is still understood of the precise mechanism by which outflows are launched and of the exact connection between outflow and accretion.
The overall objective of this project is to provide observational constraints to jet la…
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