Calendar
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MHD simulations of protostellar jets: formation and stability of shock diamonds | S. Ustamujic ( Universidad Complutense de Madrid (Spain) )
15:30
MHD simulations of protostellar jets: formation and stability of shock diamonds | S. Ustamujic ( Universidad Complutense de Madrid (Spain) )
Jun 25 @ 15:30
The early stages of a star birth are characterised by a variety of mass ejection phenomena, including outflows and collimated jets, that are strongly related with the accretion process developed in the context of the star-disc interaction. After been ejected, jets move through the ambient medium, interacting and producing shocks and complex structures that are observed at different wavelength bands.
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