Nova V Persei - a classical nova in the ``period gap''

Details Nova V Persei - a classical nova in the ``period gap'' Nova V Persei - a classical nova in the ``period gap''

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..543k&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 5

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2

Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Photometric, Polarimetric, And Spectroscopic Instrumentation, Charge-Coupled Devices, Image Detectors, And Ir Detector Arrays

Scientific paper

We report new CCD-photometric observations of the old nova V Per. The monitoring was carried out in autumn 2001 in R and V-bands. The eclipsing light curves are presented and analyzed. The value of the orbital period derived by Shafter and Abbott [1] was corrected a little. The period of the system is in the middle of the ``period gap''. In fact a half of the stars in the ``period gap'' belongs to superhumpers.

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