Observations of Cygnus X-3 above 10(15) eV from 1979 - 1984

Astronomy and Astrophysics – Astronomy

Scientific paper

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Gamma Ray Astronomy, Gamma Ray Beams, Gamma Ray Bursts, Gauss Equation, Interstellar Radiation, Muons, Neutron Stars, Stellar Atmospheres, Stellar Magnetic Fields, Time Measurement, Variability, Cerenkov Counters, Cygnus Constellation, Neutron Beams, Stellar Physics, Stellar Radiation, X Ray Binaries

Scientific paper

The ultra high energy γ-ray source, Cygnus X-3, has been observed
more or less continuously with an array sensitive to
>1015eV primaries between 1 Jan 1979 and 31 Dec 1984. The
authors find there is evidence for time variability in the phase of
γ-ray emission over this period.

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