Plasma Magnetosphere Formation Around Oscillating Magnetized Neutron Stars

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dc.creatorAhmedov, B. J.
dc.creatorMorozova, V. S.
dc.date2009-01-08
dc.date.accessioned2026-07-07T12:32:27Z
dc.date.available2026-07-07T12:32:27Z
dc.descriptionThe notion of death line of rotating pulsars is applied to model of oscillating neutron stars. It is shown that the magnetosphere of typical non-rotating oscillating stars may not contain secondary plasma to support the generation of radio emission in the region of open field lines of plasma magnetosphere.
dc.descriptionAccepted for publication in Astrophysics & Space Science
dc.identifierhttps://arxiv.org/abs/0901.1008
dc.identifierhttp://arxiv.org/abs/0901.1008
dc.identifierdoi:10.1007/s10509-009-9978-9
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/216785
dc.subjectSolar and Stellar Astrophysics
dc.titlePlasma Magnetosphere Formation Around Oscillating Magnetized Neutron Stars
dc.typetext

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