An MHD study of SN 1006 and determination of the ambient magnetic field direction

@article{Schneiter2010AnMS,
  title={An MHD study of SN 1006 and determination of the ambient magnetic field direction},
  author={E. Matias Schneiter and Pablo F. Vel'azquez and Estela Marta Reynoso and Fabio De Colle},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2010},
  volume={408},
  pages={430-435}
}
In this work, we employ a magnetohydrodynamic (MHD) numerical code to reproduce the morphology observed for SN 1006 in radio synchrotron and thermal X-ray emission. We introduce a density discontinuity, in the form of a flat cloud parallel to the Galactic plane, in order to explain the NW filament observed in optical wavelengths and in thermal X-rays. We compare our models with observations. We also perform a test that contrasts the radio emitting bright limbs of the supernova remnant against… Expand

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