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Magnetic Reconnection Detonation in Supernova Remnants

  • Authors: Horace Zhang, Yang Gao, and Chung K. Law

2018 The Astrophysical Journal 864 167.

  • Provider: AAS Journals

Caption: Figure 1.

ZND structure of the MR detonation for the Crab Nebula. The upstream is the ISM, the Neumann layer is the compressed ISM, and the downstream is the nebula. Typical density of the ISM, shock speed, and nebula temperature are used in plotting the structure (Gao & Law 2011).

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