Plasma magnetosphere formation around oscillating magnetized neutron stars

B. J. Ahmedov, V. S. Morozova

Research output: Contribution to journalArticle

6 Scopus citations

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.

Original languageEnglish (US)
Pages (from-to)115-117
Number of pages3
JournalAstrophysics and Space Science
Volume319
Issue number2-4
DOIs
StatePublished - Feb 2009

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Plasma magnetosphere formation around oscillating magnetized neutron stars'. Together they form a unique fingerprint.

  • Cite this