Very High Energy γ-Ray Generation Near The Light Cylinder of an Axisymmetric Rotator: Cos-B Like γ-Ray Sources
1992 ◽
Vol 128
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pp. 207-208
AbstractSuper-hard γ-ray radiation spectra have been calculated. This radiation is generated near the velocity-of-light cylinder through the process of inverse-Compton scattering of relativistic electrons by thermal photons radiated by a neutron star. These calculations have been compared with observations of the Crab and Vela pulsars at 1000-GeV γ-ray energies. A correlation between γ-ray flares and those in soft (Ex ≃ lkeV) X-rays are predicted.
1996 ◽
Vol 160
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pp. 363-364
Keyword(s):
2000 ◽
Vol 177
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pp. 531-532
2012 ◽
Vol 754
(1)
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pp. 33
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Keyword(s):
2013 ◽
Vol 777
(1)
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pp. L18
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