Long-term properties of X-ray binaries in the magellanic clouds
Doctoral Thesis
2013
Permanent link to this Item
Authors
Journal Title
Link to Journal
Journal ISSN
Volume Title
Publisher
Publisher
University of Cape Town
Department
Faculty
License
Series
Abstract
Long-term variability in all types of X-ray binaries is a well established characteristic, but due to observation limitations and lack of long-term monitoring capability these variations have not been studied before in a systematic way. In this thesis, we exploit the ~ 16 yr optical light curves from the MACHO and OGLE databases, and combine these with archival XMM-Newton X-ray observations to study the long-term properties of Be/X-ray binaries and Supersoft X-ray Sources in the Magellanic Clouds.
Description
Includes abstract
Includes bibliographical references.
Keywords
Reference:
Rajoelimanana, A. 2013. Long-term properties of X-ray binaries in the magellanic clouds. University of Cape Town.