Efficient cosmic-ray production in supernova remnant G347.3-0.5

Details Efficient cosmic-ray production in supernova remnant G347.3-0.5 Efficient cosmic-ray production in supernova remnant G347.3-0.5

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002newar..46..503e&link_type=abstract

New Astronomy Reviews, Volume 46, Issue 8-10, p. 503-506.

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Broad-band models of the bright NW limb of G347.3/-0.5 give convincing evidence that the forward shock of this supernova remnant is accelerating cosmic rays efficiently, placing />25% of the shock kinetic energy flux into relativistic ions. Despite this high efficiency, the maximum electron and proton energies are well below the observed `knee' at ~1015 eV in the Galactic cosmic-ray spectrum.

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