| Autor: |
Sinitsyna, V. G., Arsov, T. P., Alaverdian, A. Y., Borisov, S. S., Mirzafatikov, R. M., Nikolsky, S. I., Sinitsyna, V. Y., Platonov, G. F., Capdevielle, J. N. |
| Předmět: |
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| Zdroj: |
International Journal of Modern Physics A: Particles & Fields; Gravitation; Cosmology; Nuclear Physics; 11/20/2005, Vol. 20 Issue 29, p7023-7025, 3p |
| Abstrakt: |
The observational data for the Galactic source Cygnus X-3 collected with the SHALON mirror Cherenkov telescope are presented. The Cygnus X-3 binary have been regularly observed since 1995 with the average γ-ray flux F (E > 0.8 TeV) = (6.8 ± 0.7) × 10-13cm-2s-1. The flux in year 2003 was (1.79 ± 0.33) × 10-12cm-2s-1. Earlier, in 1997, an increase of the flux was also observed. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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