Recording of ultrahigh-energy cosmic rays from the binary systems CYG X-1 and CYG X-3

Details Recording of ultrahigh-energy cosmic rays from the binary systems CYG X-1 and CYG X-3 Recording of ultrahigh-energy cosmic rays from the binary systems CYG X-1 and CYG X-3

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pzetf..46..249k&link_type=abstract

Pis'ma v Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0370-274X), vol. 46, Sept. 25, 1987, p. 249-251. In Russian.

Physics

Binary Stars, Cosmic Ray Showers, Point Sources, Radiant Flux Density, Energy Distribution, Muons

Scientific paper

Comsic rays with an energy of about 10 to the 15th eV from point sources were measured with an EAS facility situated 192 m above sea level. An excess of 'old' showers from Cyg X-1 during 1985-1986 was observed which amounts to 3.8 standard deviations. An analysis of data on muons with energies greater than 10 GeV in selected showers shows that, on the average, the fraction of muons in showers from Cyg X-1 and Cyg X-3 is 0.8 + or - 0.1 of that in normal extensive air showers.

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