CORDIS Project
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This project investigates the dynamics of young stellar object jets, focusing on the two-component nature of these plasma outflows. By merging theoretical models, numerical simulations, and observational data, it aims to create realistic models that explain the formation and structure of protostellar jets in star forma…
Young stellar object jets are supersonic and highly collimated plasma outflows that propagate for large distances.
Although their association to star formation is a well established fact, there are still open questions such as whether the outflow is of a disk or stellar origin, or how the jet's time variable structure is produced.
Recent theoretical arguments and observational data seem to point towards the two-component nature of protostellar jets, a scenario wherein a high mass loss rate disk…
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