Confirmation of strong magnetic field amplification and nuclear cosmic ray acceleration in SN 1006
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20031667/pdf
Reference21 articles.
1. X‐Ray Synchrotron Emission from 10–100 TeV Cosmic‐Ray Electrons in the Supernova Remnant SN 1006
2. Small‐Scale Structure of the SN 1006 Shock withChandraObservations
3. The acceleration of cosmic rays in shock fronts - I
4. Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field
5. Maximum energy of cosmic rays accelerated by supernova shocks
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