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XIV International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI2006), Weihai : Chine (2006)
TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3
V.G. Sinitsyna, T.P. Arsov, A.Y. Alaverdian, S.S. Borisov, R.M. Mirzafatikhov, F.I. Musin, S.I. Nikolsky, V.Y. Sinitsyna, G.F. Platonov, J.-N. Capdevielle1

The new galactic gamma-source (neutron star) 2129+47XR is detected at energy >0.8 TeV with flux (0.19±0.09)x10^-12 cm^2s^-1 and indices of the integral spectra are kγ=−1.12±0.06, kON=−1.28±0.07 and kOff=−1.73±0.07. The results of ten-year observation of galactic source Cygnus X-3 by SHALON mirror Cherenkov telescope are discussed. The gamma -quantum spectra and images of the sources are presented. The Cygnus X-3 binary, known for more than 20 years as a source with variable intensity have been regularly observed since a 1995. The the increase of gamma-quantum flux was observed in 1997 and 2003 years.
1 :  APC - UMR 7164 - AstroParticule et Cosmologie
Physique/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique