CC Sculptoris: a superhumping intermediate polar: CC Sculptoris: a superhumping intermediate polar

K Van Der Heyden, G A Wynn,Kim L Page,Julian P Osborne,P A Evans,A P Beardmore,Franzjosef Hambsch, R Coppejans, A A S Gulbis,Brian D Warner,Patrick A Woudt

Monthly Notices of the Royal Astronomical Society（2012）

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摘要

We present high-speed optical, spectroscopic and Swift X-ray observations made during the dwarf nova superoutburst of CC Scl in 2011 November. An orbital period of 1.383 h and superhump period of 1.443 h were measured, but the principal new finding is that CC Scl is a previously unrecognized intermediate polar, with a white dwarf spin period of 389.49 s which is seen in both optical and Swift X-ra...

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关键词

binaries: close,stars: individual: CC Scl,novae, cataclysmic variables,stars: oscillations

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