Models of X-ray and Gamma-ray Emission from Pulsars

Details Models of X-ray and Gamma-ray Emission from Pulsars Models of X-ray and Gamma-ray Emission from Pulsars

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pasb.conf...93c&link_type=abstract

"Pulsars, AXPs and SGRs observed with BeppoSAX and Other Observatories, Proceedings of the International Workshop held in Marsal

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Scientific paper

In this review paper, we present a three dimensional pulsar outer-magnetospheric gap model to explain the phase-resolved X-ray and gamma-ray spectra and the energy dependent light curves from the Crab pulsar. We also extend the outer-magnetospheric gap model to longer period pulsars including Anomalous X-ray pulsars and Soft Gamma-ray Repeaters. We speculate that some of high latitude Unidentified gamma-ray point sources are long period pulsars with large inclination angle, period P ~ (0.5-0.8) s and magnetic field log(B) ~ (12.1-12.7) if they are located sufficiently closed to us, for example located in the Gould Belt.

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