Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2349e&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
2
Scientific paper
Some 6 years ago, we proposed the `single source model' in which a local, recent supernova remnant (SNR) was responsible for the `knee' in the cosmic ray (CR) energy spectrum at ˜ 3 PeV [3]. In this paper we study the possibility of observing that SNR in gamma rays and conclude that its non-observation is due to the SNR being local and in a low density region. Furthermore, being nearby it is an extended source, o ccupying up to 40° region of the sky, and indistinguishable from the background.
Erlykin Anatoly D.
Wolfendale Arnold W.
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