ar X iv : a st ro - p h / 02 03 24 7 v 1 1 5 M ar 2 00 2 1 Kilo - Second Quasi - Periodic Oscilla - tions in the Cataclysmic Variable DW Cancri
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چکیده
Our photometric monitoring revealed that DW Cnc, which was originally classified as a dwarf nova (V = 15– 17.5), remained at a bright state of Rc = 14.68 ± 0.07 for 61 days. In conjunction with optical spectra lacking a strong He ii emission line, we propose that the object is not a dwarf nova, but a non-magnetic novalike variable. Throughout our monitoring, the object showed strong quasi-periodic oscillations (QPOs) with amplitudes reaching about 0.3 mag. Our period analysis yielded a power spectrum with two peaks of QPOs, whose center periods are 37.5± 0.1 and 73.4± 0.4 min and, furthermore, with a significant power in frequencies lower than the QPOs. DW Cnc is a unique cataclysmic variable in which kilo-second QPOs were continuously detected for 61 days. We propose two possible interpretations of DW Cnc: (i) A permanent superhumper below the period minimum of hydrogen-rich cataclysmic variables. (ii) A nova-like variable having an orbital period over 3 hours. In this case, the QPOs may be caused by trapped disk oscillations.
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تاریخ انتشار 2002