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Evidence for Muon Production by Particles from Cygnus X-3

M. L. Marshak, J. Bartelt*, H. Courant, K. Heller, T. Joyce, E. A. Peterson, K. Ruddick, and M. Shupe

D. S. Ayres, J. Dawson, T. Fields, E. N. May, L. E. Price, and K. Sivaprasad

  • School of Physics, University of Minnesota, Minneapolis, Minnesota 55455

  • High Energy Physics Division, Argonne National Laboratory, Argonne, Illinois 60439

  • *Present address: Stanford Linear Accelerator Center, P.O. Box 4349, Stanford, Cal. 94305.
  • Present address: Department of Physics, University of Maryland, College Park, Md. 20742.

Phys. Rev. Lett. 54, 2079 – Published 13 May, 1985

DOI: https://doi.org/10.1103/PhysRevLett.54.2079

Abstract

We have observed underground cosmic-ray muons, corresponding to a secondary flux of ∼7×1011 cm2 s1, at a depth of 1800 m water equivalent, which appear to be initiated by Cygnus X-3. This identification is based on both direction and phase coherence. The existence of such secondary muons conflicts with the current understanding of photon cascades and/or the nature and location of Cygnus X-3.

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