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Rodríguez-Gil, P. and Gänsicke, B. T and Hagen, H.-J. et al. (2007) SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h. Monthly Notices of the Royal Astronomical Society, 377 (4). pp. 1747-1762. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20100311-114008360

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