  We have performed a new search for DPVs of short period in the ASAS catalog
(Pojmanski, G., 1997), focusing on those stars with orbital periods between 2
to 3 days which also show variations in their brightness. From a total of 244
objects, we have found another candidate to DPV, one whose mean brightness is
gradually decreasing. By fitting a 3rd order polynomial to the mean magnitude
and then moving it to zero for a second analysis, a gradual decrease over 2500
days was revealed. During the last 1000 days of this decrease, a 42% increase
in the variation between the minimum and maximum values of the magnitude was
observed. We determined the orbital period by using the PDM IRAF software
(Stellingwerf 1978) and estimated the errors for the orbital period and long
cycle by visual inspection of the light curves phased with trial periods near
the minimum of the periodogram given by PDM.
