Gamma rays from the Crab and VELA pulsars

Details Gamma rays from the Crab and VELA pulsars Gamma rays from the Crab and VELA pulsars

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992nascp3137..221h&link_type=abstract

In NASA. Goddard Space Flight Center, The Compton Observatory Science Workshop p 221 (SEE N92-21874 12-90)

Astronomy and Astrophysics

Astronomy

Astronomical Models, Emission Spectra, Gamma Ray Astronomy, Pulsars, Pulse Duration, Spectrum Analysis, Stellar Spectra, Diagnosis, Gamma Ray Observatory, Gamma Rays, Mathematical Models, Variability

Scientific paper

Gamma ray pulsed emission from the Crab and Vela pulsars are discussed. Emphasis is placed on use of current and future Gamma Ray Observatory observations as diagnostics to examine and constrain theoretical models. Issues on the spectra and pulse profile are discussed. Specifically, the absence and possibly significant time variability of pulsed emission below 10 MeV from the Vela pulsar represents a serious challenge to current astronomical models. Theoretical implication of this 'peculiarity' is addressed.

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