Electron acceleration in young supernova remnants

Details Electron acceleration in young supernova remnants Electron acceleration in young supernova remnants

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..383r&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 383-386 (2001).

Astronomy and Astrophysics

Astrophysics

Supernova Remnants, Cosmic Rays, Radio Galaxies

Scientific paper

There is evidence for production of relativistic electrons and amplification of magnetic fields in young supernova remnants. In a recent publication we have given a model for radio emission from SN 1993J [1]. In this paper we discuss theories of electron acceleration in supernova remnants such as SN 1993J. Similarities between particle acceleration processes in supernova remnants and radio galaxies undoubtedly exist and therefore observations of radio galaxies may provide crucial insight into interpreting supernova remnants. .

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