EGRET high-energy gamma-ray pulsar studies. 1: Young spin-powered pulsars

Details EGRET high-energy gamma-ray pulsar studies. 1: Young spin-powered pulsars EGRET high-energy gamma-ray pulsar studies. 1: Young spin-powered pulsars

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...436..229t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-367X), vol. 436, no. 1, p. 229-238

Astronomy and Astrophysics

Astronomy

109

Emission Spectra, Gamma Ray Observatory, Pulsars, Sky Surveys (Astronomy), Gamma Ray Telescopes, Gamma Rays, Spectrometers, Statistical Distributions, Stellar Models

Scientific paper

As part of its ongoing survey of the high-energy gamma-ray sky, the Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory has searched for emission from spin-powered pulsars, five of which have now been detected in the energy range 30 MeV less than or = E less than or = 20 GeV. A systematic study of the all-sky survey has found no additional pulsed gamma-ray sources. The pulsar detections, coupled with the upper limits on pulsed gamma radiation from other radio pulsars, indicate that the simplest models of gamma-ray pulsars are incomplete.

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