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CSS091109:035759+102943: A candidate polar |
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| Authors: | AD Schwope B Thinius |
| 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) |
| Keywords: | stars: novae cataclysmic variables techniques: photometric X‐rays: stars |