Bibliographic Details
| Title: |
TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3 |
| Authors: |
Sinitsyna, V.G.1, Arsov, T.P.1, Alaverdian, A.Y.1, Borisov, S.S.1, Mirzafatikhov, R.M.1, Musin, F.I.1, Nikolsky, S.I.1, Sinitsyna, V.Y.1, Platonov, G.F.1, Capdevielle, J.-N.2 |
| Source: |
Nuclear Physics B Proceedings Supplement. Jan2008, Vol. 175-176 Issue 1, p544-547. 4p. |
| Subjects: |
Spectrum analysis, Particles (Nuclear physics), Nuclear physics, Physics |
| Abstract: |
The new galactic gamma-source (neutron star) 2129+47XR is detected at energy with flux and indices of the integral spectra are , and . 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. [Copyright &y& Elsevier] |
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| Database: |
Engineering Source |
