Research topics//Stars formationLast update 01-09-2006 03:53 pm / Jean-François PanisBack to topic Research topicsStars formationIt has been shown a few years ago that non-thermal energy is responsible for the inhibition of the growth of gravitational instability (M. Pérault, J.-F. Panis and collaborators in Paris Observatory). This non-thermal energy is magnetic and turbulent. J.-F. Panis in collaboration with F. Shu (University of Berkeley) is modelling the injection of non-thermal energy into magnetized molecular clouds by the supersonic jets emitted by very young stellar objects. |
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