Microburst of TeV gamma rays from the Crab pulsar

Details Microburst of TeV gamma rays from the Crab pulsar Microburst of TeV gamma rays from the Crab pulsar

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..143v&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 143 (SEE N85-33902 22-93)

Mathematics

Probability

1

Gamma Ray Bursts, Pulsars, Stellar Radiation, Cosmic Rays, Monte Carlo Method, Periodic Variations

Scientific paper

Data on Crab pulsar from atmospheric Cerenkov array at Ooty have shown emission of TeV gamma rays in the form of microbursts. These are a series of events which are unusually closely spaced in time with time separations of less than 1.5 milliseconds. The phasogram of events in the bursts when analyzed with the Crab pulsar period shows significant peaks. Data further show that the signal is at the same absolute phase as the radio peak. Monte Carlo calculations show that the probability of peaks being due to chance is very small.

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