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
Computation of the structure of a magnetized strange quark star TEXT SIZE: A A A
After a massive star explodes as a supernova, a compact remnant can be left behind. A neutron star is a kind of possible remnant from a stellar explosion. However, some astronomers recently proposed that another kind of compact object, called a strange quark star (SQS), may also exist. This article explores some properties of SQSs including their internal structure and how a strong magnetic field might affect them.
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