Broad-Band Model Spectra of Gamma-Ray Emission from Millisecond Pulsars

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dc.creatorBulik, Tomasz
dc.creatorRudak, Bronislaw
dc.date1998-10-01
dc.date.accessioned2026-07-07T02:28:09Z
dc.date.available2026-07-07T02:28:09Z
dc.descriptionWe present spectra of pulsed gamma-ray emission expected from millisecond pulsars within the framework of polar-cap models. The spectra are a superposition of three components due to curvature (CR), synchrotron (SR), and Compton upscattering (ICS) processes. The CR component dominates below $100 $GeV and the ICS component exhibits a peak at $\sim 1 $TeV. The CR component should be observable from J0437-4715 with the next generation gamma-ray telescopes, like e.g. GLAST.
dc.description4 pages Latex, 2 postscript figures, Proceedings of the 3rd INTEGRAL Workshop
dc.identifierhttps://arxiv.org/abs/astro-ph/9810007
dc.identifierhttp://arxiv.org/abs/astro-ph/9810007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13001
dc.subjectAstrophysics
dc.titleBroad-Band Model Spectra of Gamma-Ray Emission from Millisecond Pulsars
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