Very high energy gamma-quanta 1 65 TeV from the Cygnus X-3 binary

Details Very high energy gamma-quanta 1 65 TeV from the Cygnus X-3 binary Very high energy gamma-quanta 1 65 TeV from the Cygnus X-3 binary

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006nuphs.151..489s&link_type=abstract

Nuclear Physics B Proceedings Supplements, v. 151, iss. 1 [SPECIAL ISSUE], p. 489-492.

Physics

Nuclear Physics

2

Scientific paper

The results of almost ten-year observation of Cygnus X-3 point source by SHALON mirror Cherenkov telescope are presented. The galactic source Cygnus X-3, known for more than 10 years as a source with variable intensity <10-5•10cms, was regularly observed since 1995 with average gamma-quantum flux F(E>0.8TeV)=(6.8±0.7)•10cms. The flux in 2003 was (1.79±0.33)•10cms. Earlier, in 1997, an increase in the flux was also observed (1.2±0.5)•10cms. The limits on gamma-rays from Cygnus X-3, the source that results stimulated the construction of many new detectors are presented. These upper limits and SHALON fluxes are now more than a factor 100 less than the fluxes originally reported.

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