Search for steady emission of 10-TeV gamma rays from the Crab Nebula, Cygnus X-3, and Hercules X-1 using the Tibet Air Shower Array

Details Search for steady emission of 10-TeV gamma rays from the Crab Nebula, Cygnus X-3, and Hercules X-1 using the Tibet Air Shower Array Search for steady emission of 10-TeV gamma rays from the Crab Nebula, Cygnus X-3, and Hercules X-1 using the Tibet Air Shower Array

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvl..69.2468a&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 69, no. 17, p. 2468-2471.

Astronomy and Astrophysics

Astronomy

65

Cosmic Ray Showers, Crab Nebula, Gamma Ray Astronomy, Monte Carlo Method, Point Sources, Background Radiation, Power Spectra

Scientific paper

A search has been made for a steady emission of VHE or UHE gamma rays from the Crab Nebula, Cygnus X-3, and Hercules X-1 using the data obtained from June 1990 to January 1992 with the Tibet Air Shower Array. No dc excess is found from the three sources in this period. Stringent flux upper limits obtained in the 10-TeV energy region place restrictions on the acceleration process of high-energy cosmic rays near discrete point sources.

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