TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3

Details TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3 TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008nuphs.175..544s&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 175, p. 544-547.

Physics

Nuclear Physics

1

Scientific paper

The new galactic gamma-source (neutron star) 2129+47XR is detected at energy >0.8 TeV with flux (0.19±0.09)×10cms and indices of the integral spectra are k=-1.12±0.06, k=-1.28±0.07 and k=-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.

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