Dr Warren Skidmore (St Andrews)
17th October, 2001
The Recent, Rare Superoutburst of the Extraordinary Cataclysmic Variable, WZ Sagittae
WZ Sagittae is an unusual and very important dwarf nova system, it may harbour a degenerate mass losing secondary star and a weakly magnetic rapidly rotating white dwarf primary that acts as a weak magnetic propellor. Thus WZ Sge is an important system in relation to Population Synthesis studies and accretion disc physics.

I will present highlights of recent observations of WZ Sge obtained during an extremely rare superoutburst. I will discuss the implications of preliminary analysis of time resolved spectroscopy and long term photometric monitoring obtained during the course of the outburst.

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