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• W2578344590 endingPage "stx064" @default.
• W2578344590 startingPage "stx064" @default.
• W2578344590 abstract "Three dimensional magnetohydrodynamical simulations were carried out in order to perform a new polarization study of the radio emission of the supernova remnant SN 1006. These simulations consider that the remnant expands into a turbulent interstellar medium (including both magnetic field and density perturbations). Based on the referenced-polar angle technique, a statistical study was done on observational and numerical magnetic field position-angle distributions. Our results show that a turbulent medium with an adiabatic index of 1.3 can reproduce the polarization properties of the SN 1006 remnant. This statistical study reveals itself as a useful tool for obtaining the orientation of the ambient magnetic field, previous to be swept up by the main supernova remnant shock." @default.
• W2578344590 created "2017-01-26" @default.
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• W2578344590 date "2017-01-11" @default.
• W2578344590 modified "2023-10-16" @default.
• W2578344590 title "A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case" @default.
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• W2578344590 doi "https://doi.org/10.1093/mnras/stx064" @default.
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