Plasma Magnetosphere Formation Around Oscillating Magnetized Neutron Stars
arXiv:0901.1008 · doi:10.1007/s10509-009-9978-9
Abstract
The 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.
Accepted for publication in Astrophysics & Space Science
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