CC Sculptoris: A superhumping intermediate polar
Solar and Stellar Astrophysics
2015-06-11 v1
Abstract
We present high speed optical, spectroscopic and Swift X-ray observations made during the dwarf nova superoutburst of CC Scl in November 2011. 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 unrecognised intermediate polar, with a white dwarf spin period of 389.49 s 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.
Keywords
Cite
@article{arxiv.1208.5936,
title = {CC Sculptoris: A superhumping intermediate polar},
author = {P. A. Woudt and B. Warner and A. Gulbis and R. Coppejans and F. -J. Hambsch and A. P. Beardmore and P. A. Evans and J. P. Osborne and K. L. Page and G. A. Wynn and K. van der Heyden},
journal= {arXiv preprint arXiv:1208.5936},
year = {2015}
}
Comments
Accepted for publication in MNRAS; 11 pages, 19 figures