BC UMa observation by Nakajima-san Dear Colleagues, We have received nearly 6-hour observation from K. Nakajima-san (Mie, Japan). Although there existed small light variations, no clear superhumps have been recorded. However, the characterstic time-scales of the variations seem to be similar to those of other short-period SU UMa stars before superhumps actually grow. These variations may suggest that the present outburst will evolve into a genuine superoutburst, and we are witnessing its earliest stage. We have also received a successful communication of observation from H. Maehara-san (Saitama, Japan). These observations will be reviewed when the results become available. Regards, Taichi Kato VSNET Collaboration team