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Tev gamma‐ray observations of the perseus and abell 2029 galaxy clusters

Perkins, J. S.; Badran, H. M.; Blaylock, G.; Bradbury, S. M.; Cogan, P.; Chow, Y. C. K.; Cui, W.; Daniel, M. K.; Falcone, A. D.; Fegan, S. J.; Finley, J. P.; Fortin, P.; Fortson, L. F.; Gillanders, G. H.; Gutierrez, K. J.; Grube, J.; Hall, J.; Hanna, D.; Holder, J.; Horan, D.; Hughes, S. B.; Humensky, T. B.; Kenny, G. E.; Kertzman, M.; Kieda, D. B.; Kildea, J.; Kosack, K.; Krawczynski, H.; Krennrich, F.; Lang, M. J.; LeBohec, S.; Maier, G.; Moriarty, P.; Ong, R. A.; Pohl, M.; Ragan, K.; Rebillot, P. F.; Sembroski, G. H.; Steele, D.; Swordy, S. P; Valcarcel, L.; Vassiliev, V. V.; Wakely, S. P.; Weekes, T. C.; Williams, D. A.; , (IOP Publishing, 2006-06-10)

Galaxy clusters might be sources of TeV gamma rays emitted by high-energy protons and electrons accelerated by large-scale structure formation shocks, galactic winds, or active galactic nuclei. Furthermore, gamma rays may ...

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Tev gamma‐ray observations of the perseus and abell 2029 galaxy clusters