NONTHERMAL EMISSION OF SUPERNOVA REMNANT SN 1006 REVISITED: THEORETICAL MODEL AND THE H.E.S.S. RESULTS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/759/i=1/a=12/pdf
Reference42 articles.
1. The gas density around SN 1006
2. First detection of VHEγ-rays from SN 1006 by HESS
3. Fits to X-ray, radio, and TeV data for the eastern rim of SN 1006
4. Evidence of a Curved Synchrotron Spectrum in the Supernova Remnant SN 1006
5. X‐Ray Synchrotron Emission from 10–100 TeV Cosmic‐Ray Electrons in the Supernova Remnant SN 1006
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