Plasma Magnetosphere Formation Around Oscillating Magnetized Neutron Stars
classification
🌌 astro-ph.SR
keywords
magnetosphereoscillatingplasmastarsneutronappliedaroundcontain
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.