Very High Energy Emission from Pulsars

Tadashi Kifune
1996 International Astronomical Union Colloquium  
AbstractObservations of gamma rays around 1012eV (= 1 TeV) from pulsars are reviewed and the results are discussed and compared with emission at other wavelengths. Very high energy gamma rays do not appear to be modulated with the pulsar period, which suggests that a major part of the VHE emission is not from the pulsar magnetosphere.
doi:10.1017/s025292110004183x fatcat:ojarqyabkjfafmyex6jzpp4r3u