Abstract:
The 1980-1981 U, B and V observations of the eclipsing binary BZ Eridani have been presented. A new period of BZ Eri comes out to be 0. ͩ 6641703. The colour curves of the system show appreciable variations, and are indicative of intrinsic variability. The secondary minimum falls nearly at phase 0.5. Some interesting features are given. The features of BZ Eri are changing. Some light variations are visible around the p[hase of secondary minimum. The discussion reveals that BZ Eri is a complicated system.
