GRO: Studies of high energy pulsars with EGRET

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Annihilation Reactions, Computational Astrophysics, Crab Nebula, Gamma Ray Observatory, Gamma Ray Spectra, Line Spectra, Pulsar Magnetospheres, Pulsars, Stellar Physics, Astronomical Models, Gamma Ray Astronomy, Gamma Ray Telescopes, Heao 2, Pair Production, Red Shift, Spaceborne Astronomy

Scientific paper

A reported e(+/-) annihilation line from the Crab pulsar is described on in this annual report, along with a astronomical model that was investigated theoretically and that displays all of the following properties discovered about this line:very strong (approximately 1040e(+/-) annihilations/sec); redshifted (by about 70 KeV relative to mc2 = 511 KeV); and very narrow (width approximately 10 KeV). A draft of the paper based on this research entitled, 'Pair production in the magnetosphere of the Crab pulsar and a pulsed e(+/-) annihilation gamma-ray line' is included.

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