Abstract
Recent results on study of ultra high energy radiation from astrophysical compact objects using the CYGNUS* array at Los Alamos are presented. Observation of episodic emissions from Her X-1 in 1986 are described. Two bursts of radiation on UT July 24 1986 were detected showing a periodicity of 1.2357±0.0003sec with a statistical significance of ~ 2 ×10-5. The showers were found to have a muon content similar to that for hadronic showers and the energy of their progenitors were greater than 400 TeV. The characteristic muon poor feature of similar gamma ray initiated showers was not observed for the signal.
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Yodh, G.B. et al. (1989). Ultra High Energy Radiation from Hercules X-l; New Physics Above 100 TEV ?. In: Shapiro, M.M., Wefel, J.P. (eds) Cosmic Gamma Rays, Neutrinos, and Related Astrophysics. NATO ASI Series, vol 270. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0921-2_15
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