- Access by Xinjiang University
Evidence for Muon Production by Particles from Cygnus X-3
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× , 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.
References (9)
- S. Danaher et al., Nature 289, 568 (1981)
- M. Samorski and W. Stamm, Astrophys. J. 268, L17 (1983)
- J. Lloyd-Evans et al., Nature 305, 784 (1983)
- M. van der Klis and J. M. Bonnet-Bidaud, Astron. Astrophys. 95, L5 (1981)
- J. M. Dickey, Astrophys. J. 273, L71 (1983)
- N. C. Rana et al., Astron. Astrophys. 141, 394 (1984)
- T. Stanev, T. K. Gaisser, and F. Halzen, to be published
- M. Samorski and W. Stamm, in Proceedings of the Eighteenth International Cosmic Ray Conference, Bangalore, India, edited by N. Durgaprasad (Tata Institute of Fundamental Research, Bombay, 1983), Vol. 11, p. 244
- J. Bartelt et al., to be published