The radio-loud plasma in pulsars

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dc.creatorEilek, J. A.
dc.creatorArendt Jr, P. N.
dc.creatorHankins, T. H.
dc.creatorWeatherall, J. C.
dc.date2002-04-08
dc.date.accessioned2026-07-07T02:03:22Z
dc.date.available2026-07-07T02:03:22Z
dc.descriptionThe pulsar magnetosphere contains a strongly magnetized, relativistic plasma. We need to understand the physics of that plasma if we want to connect the data to the models. Our group in Socorro is mixing theory and observations in order to study the radio-loud pulsar plasma. In this paper we report on several aspects of our current work.
dc.description16 pages, 20 figures. Invited review to appear in "Neutron Stars, Pulsars and Supernova Remnants" (proceedings of Bad Honnef meeting, Jan 2002), eds. w. Becker etal, to be published by MPI
dc.identifierhttps://arxiv.org/abs/astro-ph/0204122
dc.identifierhttp://arxiv.org/abs/astro-ph/0204122
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4362
dc.subjectAstrophysics
dc.titleThe radio-loud plasma in pulsars
dc.typetext

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