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2009-09-28
V2467 Cygni as possible intermediate polar
E. SwierczynskiM. MikolajewskiT. TomovE. RaganC. GalanA. KarskaP. WychudzkiM. WiecekM. CikalaM. Lewandowski
文献摘要
We present the results of unfiltered and UBVR_cI_c band CCD photometry fast nova V2467Cyg. Our analysis of the data gives two distinct frequencies corresponding to periods of ~3.8h and ~35 min. The observed light curve of V2467 Cyg is typical for an intermediate polar.
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