The x-ray synchrotron rims in cassiopeia a narrow with energy

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SUMMARY

    A better understanding of these rims could help the authors to constrain the downstream magnetic_field structure. Current models use three physical effects to account for the existence of the synchrotron filaments in X-ray: advection (bulk motion of the plasma), diffusion (random motion of electrons at small scales), and magnetic damping (where the X-ray emission reflects the magnetic_field morphology). In the "loss-limited" models, the magnetic_field is considered constant over the width of the rim. Loss-limited models predict a narrowing of the X-ray synchrotron filaments, with a weakening of the energy . . .

     

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