Abstract
We report optical time-resolved photometry of the CRTS transient CSS091109:035759+102943. Pronounced orbital variability with a 114 min period, large X-ray variability and the IR to X-ray spectral energy distribution suggest a classification as a magnetic cataclysmic binary, a likely AM Herculis star or polar. © 2012 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.
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APA
Schwope, A. D., & Thinius, B. (2012). CSS091109:035759+102943: A candidate polar. Astronomische Nachrichten, 333(8), 717–720. https://doi.org/10.1002/asna.201211716
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