On the origin of TeV radiation of SN 1006

Abstract

We discuss the link between the nonthermal X-radiation and TeV gamma-ray emission from SN 1006, and study the capabilities of both electronic and nucleonic models for explanation of the TeV flux observed from the northeast rim of SN 1006.

To appear in Astron. Astrophys. (12 pages, 8 figures)

Cited by in corpus (7)

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• Observational signatures of particle acceleration in supernova remnants
• Measuring the cosmic ray acceleration efficiency of a supernova remnant
• The exceptionally powerful TeV gamma-ray emitters in the Large Magellanic Cloud
• A semi-analytical approach to non-linear shock acceleration
• Electron-Ion Temperature Equilibration in Collisionless Shocks: the Supernova Remnant-Solar Wind Connection
• Shock Acceleration of Cosmic Rays - a critical review