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XMM-Newton and Optical Observations of WZ Sagittae in Quiescence

Published online by Cambridge University Press:  22 February 2018

K. Mukai  and
J. Patterson
K. Mukai
Affiliation:
Code 662, NASA/Coddard Space Flight Conter, Greenbelt, MD 20771USA (mukai@milkyway.gsfc.nasa.gov) Also Universities Space Research Association
J. Patterson
Affiliation:
Department of Astronomy, Columbia University, 550 West 120th Street, New York, NY 10027USA (jop@astro.columbia.edu)

Extract

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WZ Sge- is the prototype of a subclass of dwarf novae with an extremely long recurrence period. In addition, it exhibits rapid oscillations at 27.87 s and 28.96 s. We present our preliminary analysis of XMM-Newton and optical observations taken in 2003 May, almost 2 years after the 2001 outburst.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 244
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Patterson, J., Richman, H., Kemp, J. & Mukai, K. 1998, PASP 110, 403 CrossRefGoogle Scholar
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