Author: Ferrand G. Decourchelle A. Ballet J. Teyssier R. Fraschetti F.
Publisher: Edp Sciences
E-ISSN: 1432-0746|509|issue|L10-L10
ISSN: 0004-6361
Source: Astronomy & Astrophysics, Vol.509, Iss.issue, 2010-01, pp. : L10-L10
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Abstract
If a sizeable fraction of the energy of supernova remnant shocks is channeled into energetic particles (commonly identified with Galactic cosmic rays), then the morphological evolution of the remnants must be distinctly modified. Evidence of such modifications has been recently obtained with the
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