Polarized Emission from Supernovae Remnants
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Friday 12th
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Polarized Emission from Supernovae Remnants
We present numerical simulations of Supernovae Remnants including an estimate of the acceleration of particles in the main shock by coupling the MHD code GUAHCO and "Lagrangian Macro Particles". This particles represent a non-thermal distribution component with an energy distribution that is affected by the MHD fluid. The Lagrangian Macro-Particles allows us to estimate the Stokes parameters, yielding synthetic polarimetric observations that are compared with observations.