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Cyclic brightening in the short-period WZ Sge-type cataclysmic variable SDSS J080434.20+510349.2

By S. V. Zharikov, G. H. Tovmassian, V. V. Neustroev, R. Michel, C. Zurita, J. Echevarría, I. F. Bikmaev, E. P. Pavlenko, Young- Beom Jeon, G. G. Valyavin and A. Aviles


Received —????, accepted —???? Aims. We observed a new cataclysmic variable (CV) SDSS J080434.20+510349.2 to study the origin of long-term variability found in its light curve. Methods. Multi-longitude, time-resolved, photometric observations were acquired to analyze this uncommon behavior, which has been found in two newly discovered CVs. Results. This study of SDSS J080434.20+510349.2 concerns primarily the understanding of the nature of the observed, double-humped, light curve and its relation to a cyclic brightening that occurs during quiescence. The observations were obtained early in 2007, when the object was at about V ∼ 17.1, about 0.4 mag brighter than the pre-outburst magnitude. The light curve shows a sinusoidal variability with an amplitude of about 0.07 mag and a periodicity of 42.48 min, which is half of the orbital period of the system. We observed in addition two “mini-outbursts ” of the system of up to 0.6 mag, which have a duration of about 4 days each. The “mini-outburst ” has a symmetric profile and is repeated in approximately every 32 days. Subsequent monitoring of the system shows a cyclical behavior of such “mini-outbursts ” with a similar recurrence period. The origin of the double-humped light curve and the periodic brightening is discussed in the light of the evolutionar

Year: 2008
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