Neutral particles from Cygnus X-3 above 5 X 10 to the 17th eV

Details Neutral particles from Cygnus X-3 above 5 X 10 to the 17th eV Neutral particles from Cygnus X-3 above 5 X 10 to the 17th eV

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..64.1628t&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 64, April 2, 1990, p. 1628-1631.

Astronomy and Astrophysics

Astronomy

33

Cosmic Ray Showers, Neutral Particles, X Ray Binaries, Infrared Sources (Astronomy), Radio Sources (Astronomy)

Scientific paper

The emission of neutral particles from Cygnus X-3 has been searched for at energies above 5 x 10 to the 17th eV, using data from the Akeno 20-sq-km air-shower array spanning the period December 1984 to July 1989. A 3.5 sigma dc excess is observed around the Cygnus X-3 region. This excess corresponds to a flux of (1.8 + or - 0.7) x 10 to the -17th/sq cm s above 5 x 10 to the 17th eV, in agreement with the Fly's Eye data, but not the Haverah Park data. The signals do not show any 4.8-h periodicity. Their arrival times seem to be bunched in correlation with event-rate increases observed at 10 to the 16th eV with the Akeno 1-sq-km array.

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