Conitinued outburst of NGC5128V17 (var in front of NGC 5128) YYMMDD(UT) mag observer 980126.657 121 (F. Farrell) 980130.683 103 (F. Farrell) 980202.960 107 (B. Monard) 980203.944 109 (B. Monard) The long duration of the outburst, and the linear decline, may suggest this object to be an SU UMa-type dwarf nova. Has anyone obtained spectro- scopic confirmation? Time-resolved photometry may be useful in revealing the nature of the object. Regards, Taichi Kato