Radiating Regions in Pulsar Magnetospheres: From Theory to Observations and Back

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dc.creatorUsov, Vladimir V.
dc.date1999-11-22
dc.date.accessioned2026-07-07T02:34:35Z
dc.date.available2026-07-07T02:34:35Z
dc.descriptionWe discuss plausible locations of radiating regions in the magnetospheres of pulsars and argue that the mechanisms of pulsar radiation at different frequencies are closely connected with the locations of the radiating regions, especially in the radio range. If the region that is responsible for the bulk of the non-thermal radiation at some frequency is localized in the pulsar magnetosphere then the nature of this radiation will be either determined or, at least, restricted significantly.
dc.description4 pages, to be published in proceedings of "Pulsar Astronomy - 2000 and Beyond", ASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/9911403
dc.identifierhttp://arxiv.org/abs/astro-ph/9911403
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15298
dc.subjectAstrophysics
dc.titleRadiating Regions in Pulsar Magnetospheres: From Theory to Observations and Back
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