XMM-Newton and Optical Observations of WZ Sagittae in Quiescence

Details XMM-Newton and Optical Observations of WZ Sagittae in Quiescence XMM-Newton and Optical Observations of WZ Sagittae in Quiescence

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..244m&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

2

Scientific paper

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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