SIMBAD references

2012MNRAS.427.1004W - Mon. Not. R. Astron. Soc., 427, 1004-1013 (2012/December-1)

CC Sculptoris: a superhumping intermediate polar.

WOUDT P.A., WARNER B., GULBIS A., COPPEJANS R., HAMBSCH F.-J., BEARDMORE A.P., EVANS P.A., OSBORNE J.P., PAGE K.L., WYNN G.A. and VAN DER HEYDEN K.

Abstract (from CDS):

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 1.383h and superhump period of 1.443h were measured, but the principal new finding is that CC Scl is a previously unrecognized intermediate polar, with a white dwarf spin period of 389.49s which is seen in both optical and Swift X-ray light curves only during the outburst. In this it closely resembles the old nova GK Per, but unlike the latter has one of the shortest orbital periods among intermediate polars.

Abstract Copyright: © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS

Journal keyword(s): binaries: close - stars: individual: CC Scl - novae, cataclysmic variables - stars: oscillations

Simbad objects: 22

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2021.10.18-13:51:47

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