Fine Structure of the Thermal and Non-thermal X-rays in the Sn 1006 Shell

Abstract

The North Eastern shell of SN 1006 is the most probable acceleration site of high energy electrons (up to ∼ 100 TeV) with the Fermi acceleration mechanism at the shock front. We resolved non-thermal filaments from thermal emission in the shell with the excellent spatial resolution of Chandra. The non-thermal filaments seem thin sheets with the scales of ∼ 1… (More)

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@inproceedings{Bamba2003FineSO, title={Fine Structure of the Thermal and Non-thermal X-rays in the Sn 1006 Shell}, author={Ai Bamba}, year={2003} }