Contact | Site Map | CAS

中文 Home About Us Research News People Education Publications Resources International Cooperation Join Us
Societies & Publications
RAA Introduction
New Developments in RAA
  Location:Home>Societies & Publications>New Developments in RAA
Pulsating magneto-dipole radiation of a quaking neutron star powered by energy of Alfvén seismic vibrations TEXT SIZE: A A A
Pulsars are compact remnants of exploded stars that spin and emit radiation which we receive as bursts. This article explores a possible form of radiation from pulsars that may arise from vibrations in the surface of the pulsar. The results of this article can guide researchers looking for this type of proposed radiation.
 
Copyright @2005-2015,     National Astronomical Observatories, Chinese Academy of Sciences
20A Datun Road, Chaoyang District, Beijing, China
Tel:010-64888708    E-mail: ccz@bao.ac.cn