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
Pulse profile stability of the Crab pulsar TEXT SIZE: A A A
A pulsar is a small compact remnant of an exploded star. Pulsars emit short bursts of radiation as they spin, which astronomers detect on Earth. This article describes a study of the bursts of radiation emitted by a pulsar. In particular, it scrutinizes the properties of sequential pulsar bursts in terms of burst intensity and width.
 
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