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Gamma-rays and cosmic-rays from a pulsar in Cygnus OB2

W. Bednarek
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Abstract

We argue that gamma-rays sources observed in the direction of the Cyg OB2 association in the GeV and TeV energy range are due to a pulsar which was created by a supernova a few tens of thousands years ago. The excess of cosmic rays at 10^18 eV can be also related to the appearance of this pulsar.

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BibTeXRIS

W. Bednarek. 2003-07-10. Gamma-rays and cosmic-rays from a pulsar in Cygnus OB2. https://doi.org/10.1046/j.1365-8711.2003.06997.x

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