V2467 Cygni as possible intermediate polar

Details V2467 Cygni as possible intermediate polar V2467 Cygni as possible intermediate polar

2009-09-28

arxiv.org/abs/0909.5149v3

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, 5 figures

Scientific paper

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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