Non-thermal X-ray emission from young supernova remnants
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20034554/pdf
Reference38 articles.
1. Achterberg, A. 2000, in Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas, IAU Symp. 195, ed. P. C. H. Martens, S. Tsuruta, & M. A. Weber, ASP, 291
2. Evidence for TeV gamma ray emission from Cassiopeia A
3. Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field
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2. NON-THERMAL X-RAY EMISSION FROM THE NORTHWESTERN RIM OF THE GALACTIC SUPERNOVA REMNANT G266.2–1.2 (RX J0852.0-4622);The Astrophysical Journal;2010-09-10
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