Title: V2467 Cygni as possible intermediate polar Authors: E. Swierczynski, M. Mikolajewski, T. Tomov, E. Ragan, C. Galan, A. Karska, P. Wychudzki, M. Wiecek, M. Cikala, M. Lewandowski (Version v2)
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.
Title: V2467 Cygni as possible intermediate polar Authors: E. Swierczynski, M. Mikolajewski, T. Tomov, E. Ragan, C. Galan, A. Karska, P. Wychudzki, M. Wiecek, M. Cikala, M. Lewandowski
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.