Plasma Magnetosphere Formation Around Oscillating Magnetized Neutron Stars
Abstract
Description
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
Accepted for publication in Astrophysics & Space Science