The 1000 GeV gamma ray emission from radio pulsars

Details The 1000 GeV gamma ray emission from radio pulsars The 1000 GeV gamma ray emission from radio pulsars

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..155c&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 155-158 (SEE N85-33902 22-93)

Other

Crab Nebula, Gamma Rays, Pulsars, Pulse Duration, Pulsed Radiation, Radiant Flux Density, Energy Distribution, Energy Spectra, Flux (Rate)

Scientific paper

Radio pulsars have concentrated on long observations of the Crab pulsar and showed that it emits short intense bursts and a persistent weak periodic flux at gamma-ray energies 1000 GeV. It was shown that the light curve of the persistent emission was dominated by a single peak, coincident with the position of the radio and low energy gamma-ray main pulse. The results of a more detailed analysis of the structure of this main pulse are reported following an appraisal of the timing system. It is shown that at energies 1000 GeV the duration of the main pulse is not greater than 0.4 ms, which is less than that seen at all frequencies other than radio. Flux limits for the emission of 1000 GeV gamma-rays by seven other radio pulsars are reported

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