DE CVn
T. Kato wrote in [vsnet-campaign
1259] that this binary consists of a (presumably) white dwarf and a
M-type dwarf, resembling that of a short-period pre-CV. The orbital light
curve (cf. IBVS 4486) bears strong resemblance to the enigmatic object
CW 1045+525 (cf. A&A 380, 533), which is proposed to be a secondary-
dominated dwarf nova. Observations are encouraged.