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Particle acceleration and main parameters of ultra-high energy gamma-ray binaries

✍ Scribed by Nazar R. Ikhsanov


Publisher
Springer Netherlands
Year
1991
Tongue
English
Weight
794 KB
Volume
184
Category
Article
ISSN
0004-640X

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## Abstract We discuss the possibility of observing distant accelerators of ultra high energy cosmic rays in synchrotron gamma rays. Protons propagating away from their acceleration sites produce extremely energetic electrons during photo‐pion interactions with cosmic microwave background photons.