Answers are grounded in this paper and cite their sources.
Context. The synchrotron radio morphology of bilateral supernova remnants depends on the mechanisms of particle acceleration and on the viewing geometry. However, unlike X-ray and γ-ray morphologies, the radio emission does not depend on the cut-off region of the parent electron population, making it a simpler and more straightforward tool to investigate the physics of cosmic ray production in supernova remnants (SNRs).
No takes yet. Share an insight, caveat, or question.
A 2011 study studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: