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
V551 Aur, an oEA binary with g-mode pulsations? TEXT SIZE: A A A
Variable stars are stars that appear to change their brightness over time. This article studies a star which shows characteristics of two different types of variable stars, making modeling its behavior very challenging. The data collected by this study can help astronomers better understand this unusual star system.
 
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