摘要
我们于1989年11月30日晚对PG0027+260进行了时间分辨率为108秒的高速CCD测光,得到了一条完整的光变曲线,从而确认其为激变食变星系统,轨道周期0.
A CCD light curve of the PG0027 + 260 was observed on 30 November, 1989 with the 60/,90/180 cm BAO Schmidt. The result shows definitely that the object is an eclipsing cataclysmic binary with an orbital period of 0d146.
