HS0455+8315

This is a eclipsing SW Sex star. Monitoring is interesting to check whether this object displays deep low states typical for its class, and to trigger detailed follow-up observations once the object is found in a low state. So far only on poster-papers, but we have a full paper close to be submitted.

Literature

Gänsicke, B. T., Hagen, H.-J., Kube, J., Schwarz, R., Staude, A., Engels, D., Nogami, D., Kuduz, M., 2002. HS 0455+8315: A new eclipsing novalike variable, in The Physics of Cataclysmic Variables and Related Objects, (ASP Conference Proceedings, Vol. 261, 623, B.T. Gänsicke, K. Beuermann, and K. Reinsch)

Rodriguez-Gil, P., 2005, The role of the SW Sextantis stars in the picture of CV evolution, to appear in the Proceedings of 'The Astrophysics of Cataclysmic Variables and Related Objects', Strasbourg, France, 11-16 July 2004 (ASP Conference Series, J. M. Hameury and J. P. Lasota eds.)

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