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Showing 1 to 1 of 1 for “"Pulsarwindnebel"”.

  1. Pulsar wind nebulae at high energies

    Pulsar wind nebulae (PWNe) are the most abundant TeV gamma-ray emitters in the Milky Way. The radiative emission of these objects is powered by fast-rotating pulsars, which donate parts of their rotational energy into winds of relativistic particles. This thesis presents an in-depth study of the …

    potsdam-diss Repository record for Pulsar wind nebulae at high energies (opens in a new tab)