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of the most successful leading physical dissipative process at the origin of FRBs: 'relativistically magnetized shock waves'. In such extreme environments, where magnetic fields routinely reach 10^15 G within a
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their circumstellar environment. Stellar pulsations observed at the surface of stars provide a unique means of probing their internal structure through a technique known as asteroseismology. Over the past twenty years
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doit être amélioré et porté à 20 à environ 550 nm pour répondre aux exigences du nouveau projet AMINO (Advanced Multi-spectral Imaging using Novel wavefront sensors with Optical photon-counting detectors
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