The Rest of the Story: Radio Pulsars and IR through Gamma-Ray Emission

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dc.creatorRomani, Roger W.
dc.date2002-11-04
dc.date.accessioned2026-07-07T02:06:00Z
dc.date.available2026-07-07T02:06:00Z
dc.descriptionRecent observations have detected a number of young pulsars from the power peak in the gamma-ray band to the incoherent photon peak in the optical/IR. We have made progress on the multiwavelength phenomenology of pulsar emission and beaming, but a wide variation of light curves between different objects and different energy bands makes the full story complex. I sketch here a `Unified Model' of pulsar beaming and summarize the radiation mechanisms and their interplay in outer magnetosphere models of pulsar high energy emission.
dc.description6 pages, 3 figures, to appear in proceedings of the conference "Radio Pulsars" held in Chania, Crete, Sept 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0211064
dc.identifierhttp://arxiv.org/abs/astro-ph/0211064
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5282
dc.subjectAstrophysics
dc.titleThe Rest of the Story: Radio Pulsars and IR through Gamma-Ray Emission
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