Multicolor Photometric Observations of Two Novae: DK Lac and V Per

Details Multicolor Photometric Observations of Two Novae: DK Lac and V Per Multicolor Photometric Observations of Two Novae: DK Lac and V Per

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..372..523k&link_type=abstract

15th European Workshop on White Dwarfs ASP Conference Series, Vol. 372, proceedings of the conference held 7-11 August, 2006 in

Astronomy and Astrophysics

Astronomy

Scientific paper

The results of multicolor observations of two novae -- DK Lac and V Per -- are presented. DK Lac is a non-eclipsing system which shows the "high" and "low" states. We observed a nova-like depression of the brightness for DK Lac in 2003. V Per belongs to the eclipsing cataclysmic variables, its orbital period is in the ``period gap'' between 2 and 3 hours. The orbital light curves of V Per show variability, indicating ongoing mass transfer, in spite of theoretical arguments for the cessation of mass transfer in the ``period gap''. Some information about stars in ''the period gap'' is given.

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