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XMM-Newton and Optical Observations of WZ Sagittae in Quiescence
Published online by Cambridge University Press: 22 February 2018
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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.
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- Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004
References
Welsh, W.F., Sion, E.M., Godon, P., Gänsicke, B.T., Knigge, C., Long, K.S. & Szkody, P.
2003, ApJ
599, 509
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