arXiv · 0705.3259
The Discovery of a Persistent Quasi-Periodic Oscillation in the Intermediate Polar TX Col
Abstract
We report on the detection of an ~5900 s quasi-periodic variation in the extensive photometry of TX Col spanning 12 years. We discuss five different models to explain this period. We favour a mechanism where the quasi-periodic variation results from the beating of the Keplerian frequency of the `blobs' orbiting in the outer accretion disc with the spin frequency, and from modulated accretion of these `blobs' taking place in a shocked region near the disc/magnetosphere boundary.
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N. Mhlahlo, D. A. H. Buckley, V. S. Dhillon, S. B. Potter, B. Warner, P. Woudt, G. Bolt, J. McCormick, R. Rea, Denis J. Sullivan, F. Velhuis. 2007-05-22. The Discovery of a Persistent Quasi-Periodic Oscillation in the Intermediate Polar TX Col. https://doi.org/10.1111/j.1365-2966.2007.12003.x
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