A model of unpulsed very high energy gamma rays from the Crab Nebula and pulsar

Details A model of unpulsed very high energy gamma rays from the Crab Nebula and pulsar A model of unpulsed very high energy gamma rays from the Crab Nebula and pulsar

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...379..653k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 379, Oct. 1, 1991, p. 653-658.

Astronomy and Astrophysics

Astronomy

16

Astronomical Models, Crab Nebula, Gamma Ray Astronomy, Pulsars, Emission Spectra, Gamma Ray Spectra, Stellar Radiation, Synchrotron Radiation

Scientific paper

The angular resolution of gamma-ray detectors does not allow one to separate the nebula from the pulsar in the Crab. It is generally assumed that the steady emission of gamma rays comes from the nebula. Using the 'outer magnetospheric gap' model, an alternative mechanism in which the steady emission of gamma rays could come from a compact region, a couple of light cylinder radii beyond the pulsar.

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