The spectrum of TeV gamma rays from the Crab Nebula

Details The spectrum of TeV gamma rays from the Crab Nebula The spectrum of TeV gamma rays from the Crab Nebula

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..558f&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 558-562 (1997).

Astronomy and Astrophysics

Astronomy

Pulsars, Gamma-Ray, Supernova Remnants, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The Crab Nebula has become established as the standard candle for TeV gamma-ray astronomy. No evidence for variability has been seen. The spectrum of gamma rays from the Crab Nebula has been measured in the energy range 500 GeV to 8 TeV at the Whipple Observatory. Two methods of analysis involving independent Monte Carlo simulations and two databases of observations (1988-89 and 1995-96) were used and give close agreement. Using the complete spectrum of the Crab Nebula, the spectrum of relativistic electrons is deduced and the spectrum of the resulting inverse Compton gamma-ray emission is in good agreement with the measured spectrum if the ambient magnetic field is ~25-30 nT.

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