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High Energy Neutrinos from Blazars

Published online by Cambridge University Press:  12 April 2016

R.J. Protheroe*
Affiliation:
Department of Physics and Mathematical Physics, The University of Adelaide, Adelaide, Australia5005

Abstract

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I describe a model of energetic gamma ray and neutrino emission in blazars which is consistent with most of the gamma-ray observations, and use this model to estimate the diffuse intensity of high energy neutrinos from blazars.

Type
Part 12. Outflows from YSO and AGN
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Chiang, J., et al., ApJ, 452 156 (1995).Google Scholar
Gaidos, J.A., et al., Nature in press (1996).Google Scholar
Gaisser, T.K., Halzen, F., and Stanev, T., Physics Reports, 258, 173 (1995).CrossRefGoogle Scholar
Hill, G., Astroparticle Phys. in press (1996).Google Scholar
Kniffen, D.A., et al., ApJ, 411 133 (1993).Google Scholar
Lipari, P., Astroparticle Phys. 1 195 (1993).Google Scholar
Mannheim, M., and Biermann, P.L., A&A 221, 211 (1989).Google Scholar
Mannheim, K., Astroparticle Phys. 3 295 (1995).Google Scholar
Punch, M., et al. Nature 358, 477 (1992).Google Scholar
Shakura, N.I., and Sunyaev, R.A., A&A, 24 337 (1973).Google Scholar
Szabo, A.P. and Protheroe, R.J. Astroparticle Phys. 2 375 (1994).Google Scholar
Thompson, D.J., et al., ApJS, 101 259 (1995).Google Scholar