We present time-resolved CCD photometry of V2275 Cyg 790 days after the nova outburst. The data show a 20% peak-to-peak oscillation with a period of 24 minutes. The period appears stable over the two nights of observation, but QPO can not be ruled out.
@article{arxiv.astro-ph/0401183,
title = {Rapid Variations in V2275 Cyg (Nova Cyg 2001 #2)},
author = {P. M. Garnavich and A. J. Macdonald and B. Wu and S. M. Easterday and A. J. Libal and A. Palumbo and M. A. Quinn},
journal= {arXiv preprint arXiv:astro-ph/0401183},
year = {2007}
}
Comments
3 pages, 3 postscript figures, uses ibvs2.sty, to be published in IBVS