Morphological Evidence for Azimuthal Variations of the Cosmic-Ray Ion Acceleration at the Blast Wave of SN 1006

@article{CassamChenai2008MorphologicalEF,
  title={Morphological Evidence for Azimuthal Variations of the Cosmic-Ray Ion Acceleration at the Blast Wave of SN 1006},
  author={Gamil Cassam-Chenai and John P. Hughes and Estela Marta Reynoso and Carles Badenes and David A. Moffett},
  journal={The Astrophysical Journal},
  year={2008},
  volume={680},
  pages={1180-1197}
}
Using radio, X-ray, and optical observations, we present evidence for morphological changes due to efficient cosmic ray ion acceleration in the structure of the southeastern region of the supernova remnant SN 1006. SN 1006 has an apparent bipolar morphology in both the radio and high-energy X-ray synchrotron emission. In the optical, the shock front is clearly traced by a filament of Balmer emission in the southeast. This optical emission enables us to trace the location of the blast wave (BW… 
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