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Paper: V2467 Cygni as a Possible Intermediate Polar
Volume: 435, Binaries – Key to Comprehension of the Universe
Page: 297
Authors: Swierczynski, E.; Mikolajewski, M.; Tomov, T.; Ragan, E.; Galan, C.; Karska, A.; Wychudzki, P.; Wiecek, M.; Cikala, M.; Lewandowski, M.
Abstract: We present the results of unfiltered and UBVRcIc band CCD photometry fast nova V2467Cyg. Our analysis of the data gives two distinct frequencies corresponding to periods of 3.8 h and 35 min. The observed light curve of V2467 Cyg is typical for an intermediate polar.
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